The galaxy presents as a roughly elliptical form, exhibiting a moderate degree of roundness in its overall shape. A central bulge is discernible, displaying a smooth, concentrated luminosity. Extending from the main body are faint, diffuse features, possibly indicative of spiral arms or tidal disturbances. These extensions appear subtle and lack sharp definition. There appears to be another galaxy possibly undergoing a minor merger. The color profile suggests a population of older stars and possibly dust obscuration.
