This galaxy presents as an elliptical or lenticular type, exhibiting a centrally concentrated bulge with a generally smooth appearance. The core region displays a yellowish hue, indicative of an older stellar population. There appears to be a very faint, disk-like structure extending beyond the central bulge. The galaxy's overall shape is somewhat elongated. The surrounding regions show a subtle color gradient shifting towards a blueish tone, potentially indicating the presence of some younger stars or star forming regions in the outer parts of the galaxy, although it is not a highly active star forming galaxy. There might be signs of a minor disturbance or interaction with another galaxy, however, the evidence for a recent merger is limited.
