The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The color gradient transitions from a yellowish core, potentially indicative of an older stellar population, to a bluer outer region, suggesting the presence of younger stars or ongoing star formation, though the rates appear to be low. The overall shape is round, with no obvious signs of significant tidal disturbances or major mergers. Faint extensions or minor irregularities may be present, hinting at possible past interactions, but these do not dramatically alter the overall smooth appearance.
