The galaxy presents as a single, centrally concentrated object with a generally smooth appearance. It exhibits a largely elliptical morphology, appearing quite round. Faint extensions are possibly present, but the data does not clearly show signs of spiral arms or a well-defined disk structure. There does not appear to be any evidence of major ongoing merger activity. There may be signs of minor disturbance or tidal features, but they are not prominent. Color analysis indicates a generally older stellar population within the galaxy, with less active star formation currently occurring. The object is relatively luminous, suggesting a substantial stellar mass.
