The galaxy presents as a largely featureless, elliptical morphology. It displays a relatively smooth light distribution, with a high degree of central concentration. The color profile is dominated by a yellowish hue in the central region, suggestive of an older stellar population. There is very little indication of spiral arm structure or significant dust lanes. Faint, diffuse bluer emission can be observed extending outward from the central core, indicating some level of ongoing, but possibly low-level, star formation in the outer regions. The galaxy appears generally isolated, without signs of major tidal disturbances or ongoing mergers, although minor asymmetries may be present. Its overall shape is nearly circular.
