The galaxy presents a roughly elliptical morphology, viewed at a high inclination angle. The central region exhibits a bright, concentrated core of what is probably an active galactic nucleus. Moving outward, a disk-like structure is discernible, with some evidence of spiral arm features and potentially some dust lanes visible. The overall color distribution suggests a population of both young, blue stars and older, redder stars throughout the galaxy. The outer regions appear more diffuse and irregular in shape, indicating possible tidal interactions. The central bulge is not clearly dominant. There is a subtle warping of the disk, possibly due to a minor gravitational interaction.
