The galaxy presents a distinctly elliptical morphology, appearing elongated with a cigar-like shape. A smooth profile dominates, showing little indication of spiral arms or prominent disk structures. The core region exhibits a concentrated, bright luminosity, transitioning to a dimmer periphery. Color gradients suggest a radial variation in stellar populations or dust content, with the central region displaying a yellowish hue, possibly indicative of older stars, and the outer regions exhibiting hints of bluer tones. There are no clear signs of active galactic nuclei activity visible in this image. No major disturbances are present.
