The galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical galaxy viewed at an oblique angle, or a spiral galaxy viewed edge-on. The central region exhibits a higher concentration of light, appearing a faint yellow-orange hue, possibly indicating an older stellar population or a significant dust presence. Fainter, bluish light extends from the central bulge outwards, potentially indicating the presence of younger, hotter stars within a disk. The overall structure appears relatively smooth, with no apparent spiral arms or significant disturbances. The galaxy's edges diffuse gently into the background sky, indicating a gradual decrease in stellar density. There is no visual evidence of ongoing major mergers or tidal interactions, although some faint asymmetries in the outer regions can not be ruled out. The estimated size suggests that it is a relatively average-sized galaxy.
