The galaxy presents a generally smooth, elliptical morphology, appearing largely spheroidal in shape. There is a slight elongation, but no discernible spiral arm structure. The galaxy is dominated by a bright, concentrated central bulge. The overall color profile suggests a population of older stars, consistent with a spectral shift towards the redder end of the spectrum. There may be minor asymmetry, indicating the presence of a small tidal disturbance or minor merger event in the past. The light distribution is highly concentrated, with a notable absence of extended disk features.
