The galaxy appears as a somewhat elliptical, diffuse object. Its color profile suggests an older stellar population, with a concentration of light towards the central region, likely a bulge. Faint, extended arms are barely discernible, hinting at a possible spiral structure, although these features lack distinct definition. The overall smoothness of the light distribution indicates a relatively relaxed morphology, possibly a later-type spiral or an early-type lenticular galaxy. A slight asymmetry may be present, suggesting a minor gravitational interaction or recent accretion event. No prominent dust lanes or active star-forming regions are readily apparent in the image.
