The galaxy presents as an elongated, cigar-shaped structure, likely an elliptical or lenticular galaxy viewed at a significant angle. The central region exhibits a concentrated brightness, suggesting a dense nucleus or bulge. Proceeding outward from the center, there is a gradual decrease in luminosity. 

Color variations suggest stellar populations are present. The central region presents a reddish hue, which may signify a population of older, cooler stars. The outer edges are marginally bluer, perhaps indicative of regions of younger stars and ongoing star formation. 

The galaxy appears largely undisturbed with a smooth overall morphology, showing no evidence of significant mergers or tidal interactions. There may be some subtle irregularities but these are small. There is no clear evidence of spiral arm structures or a prominent disk.
