The galaxy presents an elliptical morphology, with a centrally concentrated bulge that appears yellowish-orange in color. The outer regions of the galaxy exhibit a bluer hue, possibly indicating the presence of younger stellar populations in the disk. The overall structure appears relatively smooth, suggesting a lack of significant recent merger activity or major disturbances. There is a slight elongation to the galaxy's shape, but it is predominantly rounded in appearance. No prominent spiral arms or bar structures are immediately apparent. The galaxy does not appear to be currently undergoing a major merger, though there might be some minor disturbance from a small companion galaxy.
