The galaxy presents as a relatively smooth, elliptical structure, with a concentrated, bright central bulge indicative of an older stellar population. The color of the bulge leans towards the redder end of the spectrum. There is evidence of a fainter, bluer disk component surrounding the bulge, though it appears less prominent and exhibits lower surface brightness. The overall shape is moderately elongated. There is an indication of a possible minor disturbance in the morphology, although the system is not currently undergoing a major merger. Star formation appears to be relatively low, based on the reddish color of the galaxy.
