The galaxy appears to be a relatively compact system, exhibiting a somewhat elliptical morphology. It displays a central concentration of light that gradually decreases towards the outer regions. The color profile suggests an older stellar population, with a yellowish hue dominating the central bulge. There is faint evidence of a possible disk structure but this is subtle and not well-defined. The overall smoothness of the light distribution indicates it is most likely not undergoing any major mergers, though there may be minor disturbances in the outer edges. There's a faint blue color in what appears to be a diffuse spiral arm, which could potentially indicate ongoing star formation activity.
