The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a bright, concentrated luminosity, suggestive of a dense stellar population, likely an older population of stars due to the yellowish hue. Moving outward from the center, the galaxy displays a gradual decrease in brightness, with a diffuse halo extending along the major axis. There are hints of disk-like structures, though features are not sharply defined. Possible faint spiral arms or dust lanes are present, but the overall form appears relatively smooth. There is no strong evidence of ongoing major merging events or significant tidal disturbances.
