The galaxy presents a flattened, elongated morphology, appearing as a spindle or cigar shape. It exhibits a smooth texture, suggestive of an elliptical galaxy, although a faint disk component may be present. The primary axis is oriented vertically in the image.

The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer edges. A slight color gradient is observed, with the central region appearing more yellow-red, potentially indicating an older stellar population. The outer regions are subtly bluer, which might indicate the presence of younger stars or ongoing star formation, albeit at a moderate rate.

There is no clear evidence of spiral arms, bar structures, or prominent dust lanes. The overall appearance is undisturbed, with no significant signs of tidal interactions or recent mergers, although minor disturbances cannot be ruled out. The galaxy appears relatively isolated within its immediate environment.
