The galaxy presents an elongated, cigar-like morphology. It exhibits a dominant central bulge that appears relatively smooth and concentrated, with a noticeable redder hue compared to the surrounding regions. This likely indicates an older stellar population within the bulge. A fainter disk extends from the central bulge, displaying a bluer color. The disk appears to be inclined, presenting an edge-on or nearly edge-on view. The overall light distribution suggests an elliptical-like morphology.

A secondary, smaller region of concentrated light is observed in close proximity to the main galaxy body. This could be a satellite galaxy undergoing a merging process or a region of intense star formation within the primary galaxy. The color of this region appears significantly bluer than the central bulge of the main galaxy, suggesting a younger stellar population and ongoing star formation.
