The galaxy presents as a somewhat elliptical, likely early-type system with a centrally concentrated, bright core. The overall color profile indicates a dominant population of older stars, trending towards redder wavelengths. There's a noticeable smoothness to the light distribution, with no prominent spiral arms or distinct features discernible. The galaxy is moderately luminous, suggestive of a relatively high stellar mass. A slight asymmetry is observed in the outer regions of the galaxy, hinting at the possibility of a past or ongoing minor interaction.
