The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape appears nearly circular when viewed from our perspective. The central region exhibits a high surface brightness, gradually decreasing towards the outer edges. The color profile displays a slightly redder hue in the central bulge, shifting towards a bluer tint in the outer regions, possibly indicating younger stellar populations within the disk. There are no clear signs of spiral arms, bars, or significant dust lanes. Minor disturbances, such as faint tidal tails or asymmetries, are not obviously present within the image, suggesting relative isolation and a lack of recent major mergers. The galaxy exhibits a dominant smooth morphology, indicating a possibly elliptical classification, or a lenticular galaxy viewed face-on.
