The galaxy appears to be a relatively compact object, exhibiting a roughly elliptical morphology. A bright, concentrated central core is evident, suggesting a possible active galactic nucleus or a dense stellar population within the galactic bulge. Moving outward from the core, the galaxy displays a more diffuse and less uniform structure. There is faint evidence of what could be spiral arm fragments, although the overall structure appears somewhat disturbed and asymmetric. A faint tidal tail or stream-like feature extends away from the galaxy, hinting at a possible past interaction or ongoing gravitational disturbance with another galaxy. The color gradients across the galaxy suggest variations in stellar populations and/or dust extinction, with bluer regions potentially indicating younger stars or lower dust content compared to the redder regions.
