The galaxy presents a somewhat amorphous morphology, potentially exhibiting characteristics of an elliptical or lenticular galaxy. The light distribution appears relatively smooth, with a concentrated central bulge region. There is a slight elongation observed, suggesting it is not perfectly spherical, but rather somewhat in between round and cigar shaped.

The light profile indicates a centrally concentrated luminosity distribution, with a gradual decrease in intensity outward from the core. It appears to be undergoing some type of merging activity, possibly a major merger or a minor disturbance from a close-by gravitational interaction. The color gradient hints at regions of varying stellar populations or dust content, with a potential for recent or ongoing star formation.
