The galaxy presents as a moderately bright, somewhat diffuse object. It displays a roughly elliptical morphology, lacking any prominent spiral arms or bar structure. There appears to be a slight color gradient, with the central region exhibiting a subtly yellower hue compared to the outer regions, which appear slightly bluer. This color difference may indicate a higher concentration of older stellar populations toward the galactic nucleus. The overall appearance suggests that the galaxy is relatively smooth, although it is possible there are some minor irregularities or disturbances present, they are not clearly seen. There is no apparent evidence of a major ongoing merger or strong tidal interactions with other galaxies.
