The galaxy presents as a smooth, elongated structure. Its overall morphology appears relatively undisturbed with no obvious signs of tidal tails, plumes, or strong asymmetries indicative of recent major merger activity. The central region exhibits a concentrated, bright yellowish color. This central color suggests an older stellar population. Extending outwards from the core, the galaxy becomes fainter with a redder hue, implying a possible decrease in the average age of stars or increased dust extinction in the outer regions. The shape is cigar-like or prolate, with a clear major axis that is much longer than its minor axis. There is no clear evidence of spiral arms or prominent disk-like features.
