The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. There is little to no evidence of spiral arm structure or distinct dust lanes. The object appears to be elongated, deviating from a perfectly circular shape; the galaxy is likely viewed at an angle. The overall color profile indicates a presence of older stellar populations, with a predominantly red-yellow hue. Star formation rates are likely low. There is no apparent major disturbance in the galaxy's form, suggesting it is not undergoing a major merger. The light is relatively consistent across the galaxy, suggesting uniform distribution of the stellar population.
