The galaxy presents an elongated, cigar-shaped morphology, with an apparent lack of spiral arm structures. It appears relatively smooth in texture, with a concentrated central region that fades gradually towards the edges. The central region exhibits a brighter, more intense glow, which is consistent with a high density of stars or active galactic nucleus. The color profile is indicative of a greater intensity in shorter wavelengths (green), suggesting a population of younger stars or active star formation. There is no clear evidence of significant tidal disturbances or ongoing mergers, although subtle irregularities might be present.
