This galaxy appears to be a flattened system, with an elongated, cigar-like morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a substantial stellar population and potentially an active galactic nucleus. Fainter, diffuse structures extend outwards from the central region. Color gradients indicate differences in stellar populations or dust content across the galaxy. The lack of clearly defined spiral arms and the relatively smooth texture suggest that the system is likely an early-type spiral galaxy or a lenticular galaxy. There may be a minor disturbance in the galaxy.
