The galaxy presents as a cigar-shaped system, elongated along its major axis. Its overall light distribution appears relatively smooth, lacking prominent spiral arms or distinct structures. The central region exhibits a slightly brighter intensity compared to the outer regions, suggesting a possible concentration of stars towards the galactic nucleus. A subtle color gradient is observed, transitioning from a bluer hue at one end to a slightly redder tone at the opposite end. This color variation may indicate variations in stellar populations or dust content along the galaxy's length. There is no apparent central bulge. There is some evidence of tidal disturbance. Overall, the galaxy appears to be a relatively isolated system, possibly an elliptical galaxy or a highly inclined spiral galaxy.
