The galaxy presents an elliptical morphology, elongated along its major axis. The central region exhibits a bright, concentrated core suggesting a high stellar density, possibly indicating the presence of a supermassive black hole. The light distribution appears relatively smooth, with a decreasing gradient extending outward from the core.

Color gradients are visible. The central region displays a yellowish hue, which may indicate an older stellar population. The outer regions show hints of bluer colors, which could be associated with younger, hotter stars within areas of ongoing or recent star formation.

There are indications of possible minor disturbances or asymmetries in the outer disk, but there is no clear evidence of a major ongoing merger or significant tidal interaction. The galaxy appears relatively isolated, without any immediately apparent companion galaxies causing significant gravitational disruption. Overall, the galaxy seems to be an elliptical galaxy undergoing some star formation.
