The galaxy presents an elongated, cigar-like morphology. Its core region exhibits a bright, concentrated luminosity, suggestive of a high stellar density or active galactic nucleus. Surrounding the core, we observe a less intense, diffuse halo. Faint hints of spiral structure or extended features appear to be present, however, these are not clearly defined. The overall color appears reddish, potentially indicating a population of older stars, dust obscuration, or a redshifted spectrum. There is a subtle color gradient across the galaxy.
