The galaxy presents as a relatively smooth, disk-like structure, seen at an oblique angle. A bright, moderately concentrated central bulge dominates the galaxy's core, exhibiting a yellowish hue. The spiral arms, if present, are tightly wound and not clearly delineated, appearing more as a general disk component surrounding the bulge. The galaxy's outer regions gradually fade into the background sky, suggesting a diffuse halo. The overall shape appears to be somewhere between round and elongated. There is no clear evidence of major mergers or significant tidal disturbances, although some minor irregularities may be present. Star formation appears to be moderate.
