The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a fairly regular morphology, with minimal signs of significant disturbances or ongoing merger activity. The galaxy's light profile suggests a gradual decline in brightness from the center outwards. There is some visual evidence of faint, extended structure surrounding the main body of the galaxy, but the diffuse nature of the light makes it difficult to determine if this is a halo or tidal feature. The color suggests a population of older stars, typical of elliptical galaxies, with a generally reddish hue and a lack of prominent blue regions indicative of active star formation.
