The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth morphology. The central bulge is prominent and appears relatively bright and concentrated. There is a hint of a disk-like structure, although it is not well-defined. The overall color gradient suggests a population of older stars, with a yellowish-red hue dominating. There are signs of possible interactions or minor disturbances. A possible merger with a smaller companion is visible. A distorted light distribution or tidal features may be present. Star formation seems minimal within the galaxy itself, indicative of a relatively quiescent system.
