The galaxy exhibits a moderately disturbed morphology, with a discernible disk-like structure tilted relative to our line of sight. The central region presents a bulge component, appearing somewhat elongated. The overall color gradient suggests a composite stellar population, with a concentration of older, redder stars in the bulge and a bluer population distributed throughout the disk, particularly at the edges. There is evidence of ongoing star formation in localized regions, indicated by the presence of bright blue and green knots within the disk. Faint tidal features, possibly indicative of a past or ongoing interaction, extend outwards from the galaxy's main body. There may be slight indications of merging with another galaxy, either still undergoing the process or after the interaction has occurred.
