The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. The visible light appears to be dominated by older stellar populations, indicated by the reddish-yellow hue. The galaxy displays a relatively high surface brightness concentration towards the center, with a gradual decrease in brightness outward.

There are notable irregularities in the galaxy's shape, suggesting a possible interaction or merger event. Distinct luminous clumps are embedded within the galaxy's overall structure, appearing offset from the main central body. This could indicate ongoing tidal disruption of smaller galaxies or remnants from a past merger.

The galaxy is moderately elongated, with a position angle deviating noticeably from a perfect circle, and exhibits a degree of asymmetry in its overall distribution of light. This further supports the possibility of recent or ongoing dynamical activity influencing its morphology.
