The galaxy presents a complex morphology, appearing to exhibit characteristics of both a spiral and an elliptical type. A concentrated, bright central bulge dominates the galaxy's core, with a distinct bluish hue indicating the presence of younger, hotter stars. Extending from one side of the central bulge is a faint, elongated arm-like structure, suggestive of a spiral arm, exhibiting a yellowish to reddish tint, indicating a population of older stars. The rest of the galaxy has a generally smooth, rounded appearance. There is a slight asymmetry in the outer regions, which could be attributed to potential tidal interactions or minor disturbances, but it is mostly quiescent. Overall, the galaxy presents a mixed morphology, potentially representing a transitional stage between a spiral and elliptical galaxy, or the aftermath of a minor merger event.
