The galaxy presents a complex morphology, exhibiting characteristics of both a smooth elliptical structure and a more disturbed, possibly merging system. The central region displays a relatively smooth, concentrated light distribution, suggesting an older stellar population and/or a bulge component. This area appears roughly circular in shape.

However, a distinct feature is observed extending from this central region, exhibiting a more elongated and less uniform structure. This feature appears to display a color gradient, transitioning from a yellow-red hue closer to the central region to a more diffuse, blueish coloration farther away. The extension seems to have some irregularities.

The presence of this extended structure, along with the color gradient and the potential disturbances in the overall morphology, suggests a possible interaction or merger event. Alternatively, the extended feature may represent a tidal tail resulting from a gravitational interaction, or a disk galaxy undergoing tidal disruption. Further spectroscopic analysis would be required to confirm these hypotheses and determine the precise nature of the galaxy's composition and dynamics.
