The galaxy presents as a relatively smooth, elliptical or lenticular structure. It appears roughly round, with a concentration of light toward the center, suggesting a substantial bulge component. The galaxy exhibits a color gradient, transitioning from a more yellow-orange hue in the core to a slightly bluer color in the outer regions. This color variation may indicate a difference in stellar populations, with older, redder stars dominating the central bulge and a possible presence of younger, bluer stars in the outer regions. There are some disturbances possibly due to a minor interaction with a neighboring galaxy or other tidal disruption. Overall, the morphology is suggestive of a galaxy undergoing some form of galactic evolution, showing a generally aging stellar population.
