The galaxy exhibits a generally smooth morphology, with an elliptical appearance. The central bulge is bright and concentrated, appearing more yellow in color, possibly indicating an older stellar population dominating the core. Surrounding the bulge is a fainter, bluer halo or disk-like component. The blue hue suggests the presence of younger, hotter stars. This outer region appears less defined, lacking prominent spiral arms or distinct features. The overall shape leans towards round, though some elongation is present, suggesting a slight deviation from a perfect sphere. There is no obvious evidence of significant mergers or tidal disturbances, though subtle asymmetries cannot be ruled out from this image alone.
