The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, appearing reddish in color, suggesting an older stellar population and minimal ongoing star formation in the core region. Surrounding the central bulge is a more diffuse halo, with a blue-green hue, indicating the presence of some younger, hotter stars, though the overall star formation rate appears relatively low. There are hints of a faint disk-like structure, but the galaxy lacks prominent spiral arms or other distinct features. The overall shape is largely round, with no obvious signs of major disturbances or ongoing mergers, though minor disturbances cannot be entirely ruled out given the slight asymmetry in the outer regions.
