The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color appears yellowish-orange, suggestive of an older stellar population and a lack of significant ongoing star formation. There is a subtle hint of asymmetry or disturbance in its shape, with a slight extension or tidal feature emanating from one side. This could be indicative of a past or ongoing interaction with another galaxy, or a minor internal disruption. The galaxy appears somewhat compact, with a fuzzy or diffuse halo surrounding the core. There are no distinct spiral arms or dust lanes visible.
