The galaxy presents as a flattened, disk-like structure, viewed at an oblique angle. A prominent central bulge exhibits a yellow-orange hue, suggestive of an older stellar population. Fainter, bluer regions are visible in the outer disk, potentially indicative of more recent star formation. The overall smoothness of the galaxy implies that it is most likely an early-type spiral galaxy. There is no strong evidence of ongoing major mergers or significant tidal distortions, although some subtle irregularities in the outer regions cannot be ruled out, suggesting a possible minor interaction in its past. The absence of well-defined spiral arms further supports its classification as an early-type spiral. The galaxy appears relatively isolated, with no other immediately apparent large companions.
