The galaxy presents a morphology consistent with a spiral structure, though somewhat disturbed. The central bulge appears moderately sized. Faint spiral arms emanate from the core, displaying a relatively tight winding pattern. The overall color suggests a relatively low rate of recent star formation. There is evidence of a possible tidal tail extending from the main galactic body, suggesting a past or ongoing gravitational interaction. The central region exhibits a brighter, compact core possibly indicating an active galactic nucleus, or a high concentration of stars. The galaxy's disk is inclined at an angle relative to our line of sight, allowing a partial view of its spiral structure. Some asymmetry is present in the outer regions, hinting at possible ongoing mergers or interactions.
