The galaxy exhibits a generally smooth morphology, appearing somewhat elongated or cigar-shaped. The central region presents a brighter, more concentrated luminosity, suggesting a higher stellar density or possibly an active galactic nucleus. The light distribution transitions gradually from the core to the outer regions. There is a subtle color gradient, with the central part displaying a bluer hue, potentially indicating a younger stellar population or ongoing star formation. The periphery seems slightly redder, which could reflect an older stellar population. Overall, the galaxy does not display prominent spiral arms or a well-defined disk structure but seems to be more akin to an elliptical or lenticular galaxy experiencing some form of activity or disturbance. There is a suggestion of minor disturbances or tidal features on either side.
