The galaxy presents as a relatively smooth, elliptical morphology. The light profile exhibits a centrally concentrated bulge that dominates the overall luminosity. There appears to be very little, if any, visible disk structure. The galaxy has a generally round appearance, with only a slight elongation. There is no evidence of significant tidal features or distortions suggestive of a recent major merger event. The galaxy core is bright, with the overall color indicative of an older stellar population, consistent with low star formation rate. Some subtle, low-level asymmetries or minor disturbances may be present.
