This galaxy appears to be a relatively compact object. It presents as a somewhat amorphous, roughly elliptical form with a bright central concentration of light. The overall color profile appears bluer towards the center, suggesting a population of hotter, younger stars or possibly active galactic nucleus activity. There's some indication of a faint, extended halo or envelope surrounding the main body of the galaxy, though it's diffuse and difficult to discern distinct features. A slight asymmetry in the outer regions may hint at a minor gravitational interaction or recent merger event. Given its morphology and color, this galaxy could be classified as an early-type spiral or a lenticular galaxy undergoing some form of disturbance.
