The galaxy presents as a generally smooth, elliptical-like structure, with a concentrated central bulge. Its overall shape leans towards being in between round and cigar-shaped, not perfectly spherical nor elongated. There appears to be a faint disk. The color profile suggests an older stellar population. There is no obvious presence of ongoing major mergers or significant tidal distortions, with most classifications suggesting a non-merging state. The color profile of this galaxy leans towards redder wavelengths, indicating the presence of older stars. 
