The galaxy presents as an elongated, somewhat irregular object. It exhibits a central concentration of light, suggesting a bulge or core region. The color distribution shows a gradient, with the central region appearing more yellow/white, potentially indicative of an older stellar population. The outer regions appear slightly bluer, which might be a sign of ongoing or recent star formation. There is an asymmetry or faint tail-like structure extending from one side of the galaxy. Overall, the galaxy appears to be a relatively massive system and exhibits some signs of potential interaction or past merger activity.
