The galaxy exhibits a morphology that appears to be disturbed or undergoing interaction. A significant portion of the galaxy presents a smooth, centrally concentrated light profile, suggestive of an elliptical or spheroidal component. A faint, elongated feature extends from the main body, possibly a tidal tail or disrupted arm, indicating gravitational interaction with another galaxy or recent merger activity. The color distribution shows a gradient, with the central region appearing more yellow-red, potentially indicating an older stellar population. There is a knot of bluer emission, which might represent a region of active star formation, towards the edge of the galaxy in the direction of the elongated feature.
