The galaxy presents as a smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge that dominates its overall luminosity. There is little indication of distinct spiral arms or complex features usually associated with spiral galaxies. The color profile suggests an older stellar population, with a reddish-yellow hue implying the presence of evolved stars and a relative lack of ongoing star formation. The galaxy appears elongated, with a clear major axis orientation. The isophotes are generally smooth and consistent with an elliptical morphology, although there might be subtle deviations hinting at possible tidal interactions or past mergers. The overall appearance suggests a relatively evolved galaxy in terms of its morphological type and stellar population.
