The galaxy presents as an elliptical morphology, generally smooth in appearance with a high degree of central concentration. The color index suggests a population of older stars, likely with a low ongoing star formation rate. The overall shape approximates an ellipse, exhibiting a moderate degree of elongation. There is no obvious evidence of strong tidal interactions or major mergers; any disturbances present are likely minor or undetectable at this resolution. The galaxy's spatial extent is relatively compact, appearing well-defined and isolated.
