The galaxy presents as a roughly elliptical or lenticular structure. The central region exhibits a high degree of smoothness, with a concentration of light suggesting a significant bulge component. Extending outward from the core, there appears to be a faint, diffuse halo or disk-like component. The overall color is consistent with an older stellar population, displaying yellow and reddish hues with a small amount of blue possibly indicating some star forming regions. There is a high probability of a merger event that has taken place and may be responsible for some minor disturbances.
