The galaxy presents as an elongated, cigar-shaped structure, indicating a likely elliptical morphology or a highly inclined disk galaxy. The central region exhibits a concentrated luminosity, suggesting a substantial stellar population and potentially a supermassive black hole at the galactic nucleus. Color gradients are present, with a reddish hue dominating the central bulge, possibly due to older, cooler stars. Fainter bluish components extend outwards from the core region, which may indicate younger stellar populations or regions of active star formation. There appears to be some subtle distortion in the morphology, perhaps indicating tidal interactions or past minor merger events.
