The galaxy presents as a centrally concentrated, relatively smooth object. Its dominant color is a yellow-orange hue, suggesting an older stellar population. The overall shape appears elliptical, with no apparent spiral arm structures or significant dust lanes visible. There is a slight elongation present, but it generally appears quite round. The smooth light distribution indicates the absence of recent major mergers, though a subtle irregularity in the outer regions hints at possible minor tidal interactions or past accretion events. The lack of bright blue regions suggests a low star formation rate within the visible area.
