This galaxy presents as a smooth, cigar-shaped system. The core exhibits a concentrated, bright luminosity, suggesting a high density of stellar populations or potentially an active galactic nucleus. There are no immediately obvious spiral arm structures or dust lanes visible in this image, which is consistent with an elliptical morphology. The color profile is relatively uniform across the galaxy, with a generally reddish hue. This reddening is indicative of an older stellar population, possibly with ongoing star formation. No signs of major mergers or significant tidal disturbances are apparent.
