The galaxy presents as a relatively smooth, centrally concentrated object. It displays a somewhat elliptical morphology, appearing more rounded than elongated. The color gradient suggests an older stellar population, with the central region exhibiting a yellowish hue, possibly indicating a concentration of older, redder stars. The outer regions transition towards a bluer color, although the degree of blue enhancement is moderate, implying some presence of younger stars but not dominant. There seems to be a disturbance, potentially a minor merger event happening. There seems to be light emitting from the central region which indicates the active galactic nucleus may be active. Overall, the galaxy's characteristics point towards a relatively evolved system, possibly in transition from a spiral to an elliptical morphology, or undergoing a minor merger event.
