The galaxy presents as an elongated, cigar-shaped structure, oriented approximately horizontally within the image frame. A color gradient is observable, with the central region exhibiting a yellowish-white hue, suggesting a population of older stars. The outer regions appear fainter and slightly bluer, hinting at the presence of younger stellar populations.

There is little to no indication of spiral arm structure or prominent dust lanes. The galaxy's overall morphology is relatively smooth, lacking any significant features indicative of active star formation or major disturbances. There is a slight asymmetry in the distribution of light, with a gradual decrease in luminosity from the center outwards, the galaxy appears to be an edge-on view of a disk galaxy with a central bulge and a smooth disk.

Based on the apparent color and smooth morphology, this galaxy is likely composed primarily of older stars, with relatively low levels of current star formation.
