The galaxy presents as a relatively smooth, disk-shaped object with a central bulge. The core appears bright and yellowish, indicative of an older stellar population. Surrounding the core, a fainter, bluer disk is visible, likely containing younger stars and some ongoing star formation. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated rather than perfectly circular. There are no obvious signs of strong tidal interactions or major mergers, although subtle distortions within the disk could suggest minor disturbances or past interactions. The overall morphology leans towards that of a late-type spiral galaxy, though the smoothness and prominence of the bulge also suggest characteristics of an early-type spiral, possibly an Sa or Sb classification.
