The galaxy presents as a relatively small, elliptical or lenticular-shaped object, with an estimated effective radius of roughly 4.5 arcseconds. The central region exhibits high surface brightness, appearing nearly uniform and concentrated, suggesting an older stellar population. Moving outwards from the core, the light distribution decreases gradually, though the outer edges are poorly defined. There are no obvious spiral arm structures present and the galaxy appears primarily smooth in appearance. There appears to be possible tidal disruption around the central region, which could indicate a possible minor merger event. There does not appear to be any indication of a merger, as the galaxy appears to be largely unperturbed. There is a hint of bluer colors around the outside of the galaxy, but these are very faint and difficult to see. The object is likely relatively quiescent with little active star formation. 
