The galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type. It exhibits a roughly circular morphology with a bright, unresolved core, suggesting the presence of an actively accreting supermassive black hole or a dense stellar nucleus. The light profile diffuses outward from the core, transitioning into a more extended, fainter halo. The galaxy displays a bluer color in its central regions, possibly indicative of ongoing star formation. The outer regions appear redder, which might be a result of an older stellar population dominating these areas. There's no clear evidence of spiral arms, bars, or significant dust lanes. Overall, the galaxy appears to be largely undisturbed.
