The galaxy presents an elliptical morphology, exhibiting a relatively smooth, centralized light distribution. It is characterized by a generally round shape, with a slight elongation. The central region displays a higher concentration of light, suggestive of a galactic bulge. The overall color appears to be slightly blue, which could indicate ongoing star formation, though the low rate suggests that the stellar population may be relatively old. There is no evidence of major disturbances, such as tidal tails or strong asymmetry, but there are some slight, possibly minor disturbances.
