The galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent, relatively bright central bulge dominates the structure. The disk component is visible as a flattened structure extending outwards from the bulge, with some obscuration along the central plane, potentially indicating the presence of dust lanes. The bulge exhibits a somewhat rounded morphology. There does not appear to be any significant evidence of strong tidal features or ongoing major mergers, however some signs of minor disturbances cannot be ruled out. Overall, the galaxy appears relatively undisturbed. The colour of the bulge appears more yellow/red compared to the disk, potentially indicating an older stellar population. The galaxy appears moderately luminous.
