The galaxy presents as a relatively smooth, elliptical structure. The central bulge exhibits a bright, concentrated luminosity, suggestive of a high stellar density. The overall shape is moderately elliptical, appearing more oblate than spherical. There is faint evidence of a disk-like structure surrounding the central bulge. The color profile indicates a slightly redder hue within the bulge, potentially indicating an older stellar population, while the outer disk shows bluer tones, possibly indicating ongoing star formation. There are no apparent signs of major disturbances, like tidal tails or strong asymmetries, indicating a lack of recent major mergers. Minor disturbances may be present in the outer disc region. Overall, this galaxy appears to be a fairly typical elliptical galaxy with potential indications of a small disk component and minor interactions.
