This galaxy presents a somewhat disk-like morphology, although the structure is more difficult to discern due to its observed smoothness. A central bulge is apparent, characterized by a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy exhibit a slightly bluer coloration compared to the core, hinting at the presence of younger stars and ongoing, though perhaps subdued, star formation. Some irregularities in the disk's overall form and light distribution are present, possibly indicating minor gravitational interactions or internal disturbances. Evidence of a substantial merger is not immediately apparent, but subtle tidal features may be present upon closer examination. The overall profile indicates that it is more round than cigar shaped.
