The galaxy presents as an elongated, roughly elliptical form. A central bulge is visible, displaying a reddish-orange hue. The surrounding disk shows a less intense, somewhat mottled distribution of light with hints of greenish regions. The galaxy lacks any easily discernible spiral arm structure. The overall color profile suggests a population of older stars dominating the central regions, with hints of younger stellar populations and/or ionized gas contributing to the greenish tints in the disk. The galaxy's morphology appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions.
