The galaxy presents as an elliptical or lenticular-like structure. It has a smooth, diffuse appearance, with no obvious spiral arm features or distinct dust lanes visible in this imagery. The light is concentrated towards the center of the galaxy, gradually fading outward towards the edges, indicating a centrally concentrated stellar population. The overall color appears to be slightly redder, suggesting a population of older stars. There is a slight asymmetry, possibly due to a minor gravitational interaction or internal dynamical processes. No clear signs of on-going major merging activity or violent star formation are immediately apparent in the image. The galaxy exhibits a relatively compact size.
