This galaxy presents an elliptical morphology with a prominent central bulge. The light distribution appears relatively smooth, suggesting an older stellar population and a lack of significant recent star formation within the bulge. However, there are hints of more distinct, irregular structures, possibly spiral arms or tidal features, extending outward from the core of the galaxy. These features exhibit a bluer color, suggesting younger stars and ongoing star formation activity in these regions. This might be a result of minor mergers or interactions with other galaxies. The main body of the galaxy is more rounded in appearance, while the outer regions show some deviation from perfect elliptical symmetry. The overall color gradient suggests a complex star formation history, with an older, redder population dominating the central bulge and younger, bluer stars residing in the outer features.
