The galaxy presents as a relatively smooth, elongated structure. Its shape appears to be more cigar-shaped than circular. The central region exhibits a concentration of light, possibly indicative of a galactic bulge. The galaxy displays a blue hue, implying the presence of younger, hotter stars. There is some indication of a disk structure, though it lacks a prominent spiral arm morphology. Minor disturbances are present, though it is not a strong merging event.
