The galaxy appears to be an elliptical type, exhibiting a generally smooth, spheroidal morphology. There is a slight elongation but not a significant disk-like structure. The color is primarily yellowish-orange, suggesting an older stellar population with a relative deficiency of young, blue stars. There seems to be a lack of distinct spiral arm features or prominent dust lanes. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions, indicating a relatively smooth density profile. There are no obvious signs of major mergers or tidal disturbances, although some minor irregularities may suggest past interactions or internal dynamical processes. The overall structure appears relatively relaxed and evolved.
