The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. Its overall shape is elongated, closer to cigar-shaped than perfectly round. The central region displays a concentrated, bright core, likely indicating a high stellar density or perhaps an active galactic nucleus. The color profile suggests a mature stellar population, with a yellowish-red hue dominating the core, transitioning to slightly bluer tones in the outer regions, although these are less pronounced. No distinct spiral arms or prominent dust lanes are observed. There is no visual indication of a major ongoing merger or significant tidal disruption. A slight asymmetry could indicate a minor past interaction or internal dynamics. Given the apparent color and morphology, the galaxy likely has a relatively low star formation rate.
