The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a mostly elliptical morphology, deviating slightly from a perfect circular shape. The light distribution indicates a prominent bulge component, characterized by a yellowish-white hue, suggesting an older stellar population. A faint, bluer disk component surrounds the bulge, indicating recent or ongoing star formation, albeit at a low rate. There appears to be a small, reddish and disturbed area towards the outer edge of the disk, potentially indicating a minor interaction with another galaxy, or internal dust extinction. Overall, this galaxy appears to be a relatively massive system with a mix of old and young stellar populations and a faint, ongoing star formation.
