The galaxy presents as an elliptical morphology, with a generally smooth appearance. The light profile exhibits a centrally concentrated bulge, indicated by the peak in luminosity. The galaxy is slightly elongated, though it is mostly round in shape. There appears to be little to no evidence of spiral arm structures or significant tidal disturbances. The overall color gradient suggests the presence of an older stellar population, particularly in the central regions, which appear more yellow, potentially indicating a lack of ongoing star formation within the visible spectrum. There may be some minor interactions, but it is a small percentage.
