This galaxy exhibits a smooth, elongated morphology, appearing cigar-shaped. The primary light distribution suggests a dominant spheroidal component. There is a central concentration of light with a gradual decrease in brightness toward the outer edges. A subtle color gradient is observed, with the core appearing more yellow/orange and the outer regions showing a faint bluish tinge, hinting at potential variations in stellar populations. The galaxy shows subtle signs of possible disturbances or interactions, but presents a largely undisturbed single core, likely without a significant amount of current major merging activity. The galaxy's estimated size is fairly large, based on its measured distances.
