The galaxy appears to be disc-shaped, with a prominent central bulge. The bulge exhibits a high surface brightness, suggesting a concentrated stellar population. The disc appears relatively smooth, with only subtle indications of spiral arm structure. There seems to be some slight asymmetry in the outer regions of the disc, potentially indicative of tidal interactions or minor disturbances. Color variations are observed throughout the galaxy; the central bulge region is bluer than the outer disc, which is redder, possibly indicating younger stars and star forming regions present within the bulge. There is some low surface brightness emission extending outwards from the main body of the galaxy. Possible faint tidal features can be seen on the edges.