The galaxy presents as a primarily smooth object with a slight disk-like feature or disturbance. It exhibits a somewhat elliptical morphology, leaning towards an in-between form rather than being perfectly round or significantly elongated. The light distribution suggests a central bulge region that transitions into a less defined, fainter halo. There are visible irregularities within the halo structure, possibly indicating minor disturbances or interactions with other objects. The colour gradient indicates a predominantly older stellar population across the main body, with some evidence of bluer, possibly younger stars present in the area which could be interpreted as a weak star forming region. The galaxy does not appear to be undergoing a major merger, though there are disturbances which suggest it may be weakly interacting with another object.
