The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a bright, centrally concentrated bulge, suggesting a significant population of older stars. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy has an overall round appearance. There may be a very slight asymmetry or minor perturbation visible at the edge of the disk suggesting a possible minor interaction or disturbance. The object displays a color gradient, appearing slightly bluer in the outer regions and redder towards the central bulge.
