The galaxy presents as a relatively smooth, centrally concentrated structure, exhibiting a generally elliptical morphology. There is little evidence of significant spiral arm structure or a prominent disk. The light distribution appears to be dominated by a bulge component. The color profile is moderately red, suggesting a population of older stars. The galaxy appears relatively undisturbed, lacking any major distortions or tidal features indicative of recent major mergers. However, some minor asymmetric features could suggest minor disturbance. The estimated size of the galaxy is moderate. The galaxy's overall appearance suggests it is an evolved system with a relatively low star formation rate.
