The galaxy presents a generally smooth morphology with a dominant central bulge. It exhibits a yellow to golden hue, potentially indicative of an older stellar population and low ongoing star formation activity. The galaxy appears somewhat elliptical in shape but mostly rounded, with a slight elongation. There is a subtle hint of disk structure, though it is not sharply defined. Possible minor disturbance or interaction is suggested by the slight asymmetry in the outer regions, but no distinct tidal tails or merging features are readily apparent. Overall, the galaxy seems to be a relatively massive system at a considerable distance.
