The galaxy presents as a fairly compact, elliptical-like structure. The core region exhibits a bright, concentrated luminosity gradient, suggesting a high stellar density. The color profile shifts subtly from a yellow-white central region to a redder hue towards the outer edges, potentially indicative of an aging stellar population and diminished star formation activity in the galaxy's periphery. The overall morphology appears relatively smooth with a predominantly round shape, lacking significant features such as spiral arms or a prominent disk. There is no apparent evidence of tidal disturbances or ongoing major mergers.
