The observed galaxy presents as a somewhat elliptical, diffuse object. A bright central concentration is evident, suggesting a possible bulge component. A faint, extended halo surrounds this central region, fading into the background sky. Overall, the galaxy's structure appears relatively smooth, but there is subtle evidence of faint, irregular features, possibly indicative of minor disturbances or tidal interactions. The color profile suggests a mixture of stellar populations, with the central region appearing slightly bluer than the outer halo.
