This galaxy exhibits a generally smooth, elliptical morphology. The central bulge appears relatively bright and concentrated, with a color profile shifting towards the redder end of the spectrum. There is a gradual decline in luminosity extending outwards from the central region. The outer regions show an extended halo of diffuse light. There is no significant visual evidence of spiral arm structures or active star formation regions. The overall appearance suggests a relatively evolved galaxy, potentially dominated by an older stellar population.
