The galaxy presents an overall elliptical morphology. The light distribution is concentrated toward the central region, with a gradual decrease in intensity outwards. The core region displays a yellowish hue, potentially indicative of an older stellar population. There is a slight flattening to the elliptical shape, hinting at possible rotational support. The outer regions seem to have some faint and diffuse features, with a slight blue tinge, possibly indicating some areas of ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of tidal tails or major mergers.
