The galaxy presents as a relatively smooth, lenticular structure with a notable absence of distinct spiral arms. Its overall form appears more elliptical than circular, showing an intermediate ellipticity. The central bulge region is prominent and diffuse, exhibiting a gradual decline in luminosity towards the outer edges. There is a subtle hint of a disk-like structure, but it lacks the well-defined features of a spiral galaxy. The galaxy's color appears predominantly redder than the background, which indicates a population of older stars and a diminished rate of ongoing star formation. There are no prominent dust lanes visible, further supporting this observation. There are a few hints that there may be a minor disturbance within the galaxy itself, but it is largely undisturbed.
