The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, suggesting a dominant spheroid component. The core region is bright and compact, with light gradually decreasing outwards. The galaxy appears nearly circular in projection, with no obvious signs of a disk structure or spiral arms. There are only very minor, if any, disturbances in its structure. The color profile is relatively uniform, with a slight bluer hue toward the center and a redder tone in the outer regions. The apparent smoothness and color suggest a stellar population dominated by older stars, with ongoing star formation at a slow rate.
