The galaxy exhibits a generally smooth morphology, appearing as a flattened spheroid. There is a bright, concentrated central region, possibly indicative of a nucleus or bulge. A slightly fainter disk is visible extending outwards from the central region, with a notable elongation along one axis. The disk appears primarily blue, which may indicate a population of younger, hotter stars. There are some features that suggest the possibility of minor tidal disturbances or interactions, like a very slight warp in the disk's shape or low-level asymmetries in the surrounding halo. There may be faint, diffuse extensions or tidal tails, though they are not highly prominent. There are also hints of a small, red area along the plane of the disk that may be the result of dust. Overall, the galaxy shows characteristics of a relatively undisturbed disk galaxy with a notable bulge.
