The galaxy appears as a centrally concentrated, relatively smooth elliptical. It exhibits a roughly circular morphology with a high degree of central light concentration that decreases gradually outwards. The color profile shows a dominance of yellow-red hues towards the center, indicative of an older stellar population, with slightly bluer components in the outer regions. There is no evidence of spiral arms, bars, or significant dust lanes. No signs of recent major mergers or tidal disturbances are visible. The overall appearance suggests a mature galaxy dominated by evolved stars with a relatively low star formation rate.
