The galaxy appears to be elliptical, with a smooth, concentrated light profile. The central bulge is prominent and exhibits a yellowish hue, indicating a population of older stars. There's a gradual decrease in light intensity moving outwards from the core. The overall shape is roughly circular, with no distinct features such as spiral arms or prominent dust lanes visible. The galaxy does not show any obvious signs of recent merger activity or tidal disturbances. The color gradient suggests a possible lack of ongoing star formation, which is consistent with a more evolved stellar population.
