The galaxy presents an elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. There appears to be minimal evidence of spiral arm structure or prominent dust lanes. The color profile suggests an older stellar population, with a yellow-red hue dominating the central bulge and extending outwards. The galaxy does appear to be fairly well-formed, with only minor disturbances to its form based on its roundish profile. The galaxy exhibits a minor amount of star formation within it. It has a low star formation rate and a large mass which implies a fairly high mass to light ratio.
