The galaxy presents as an elongated structure, appearing largely smooth with a concentrated central bulge that exhibits a yellowish hue. This core transitions into a more diffuse, extended halo with a slightly reddish color. The overall shape indicates a possible classification as an elliptical galaxy. No distinct spiral arms or significant dust lanes are discernible. The light distribution suggests a relatively evolved stellar population, as inferred from the redder color of the halo and the yellowish bulge. The galaxy seems to be relatively isolated, exhibiting no obvious signs of recent or ongoing major merger activity or tidal disturbances, though a very subtle asymmetry cannot be completely ruled out. The galaxy has a small estimated star formation rate.
