The galaxy presents a primarily smooth appearance, suggesting it is likely an elliptical or lenticular type. It is largely spheroidal, but not perfectly round, with a slight elongation visible. There may be very faint, subtle disk-like feature, but they are not prominent. The central region is brighter and yellower in color, indicating a concentration of older stars. Moving outward from the center, the color shifts to a bluer hue, possibly indicating ongoing or recent star formation in the outer regions. There appears to be some minor disturbances in the outer regions of the galaxy, hinting at a possible past interaction or minor merger.
