The galaxy presents a generally smooth morphology. It appears approximately elliptical in shape, exhibiting a moderate degree of ellipticity. Color gradients are subtle, but the central region exhibits a yellower hue, suggesting a population of older stars. The outer regions are somewhat bluer in comparison, which could indicate pockets of more recent star formation, although the overall star formation rate appears low. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy does not show any obvious signs of a major ongoing merger or tidal disruption, although there is a slight asymmetry in the shape, suggesting a possible minor interaction in its past.
