The galaxy presents as a relatively smooth, elliptical or lenticular system, exhibiting a notable lack of distinct spiral arm structure. The overall color is yellowish-orange, suggesting a population of older stars. The galaxy appears moderately elongated, with the ratio of its major to minor axis being approximately 3:1. There is a central bulge, which is bright and concentrated, with a smooth transition into the outer regions. There are no obvious signs of significant dust lanes or active star formation. Possible very minor disturbances could be occurring due to the slight irregularities on the edges of the disk.
