This galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated core, suggesting a high stellar density, potentially an aging stellar population. Fainter and diffuse light extending from the core is observed. The outer regions display hints of spiral structure or tidal debris, evidenced by subtle color variations. The overall color of the galaxy appears redder, which might indicate older stellar populations and/or significant dust obscuration. There is no evidence of a recent major merger, but signs of potential tidal disturbances may indicate past or ongoing interactions with smaller galaxies.
