The galaxy presents as a relatively face-on spiral galaxy with a bright central bulge. The disk appears smooth with evidence of flocculent spiral arm structure. A slight blue tint is present in the disk, suggestive of ongoing star formation. The bulge appears more yellow, possibly indicating an older stellar population. The galaxy's overall shape is elliptical, with a major to minor axis ratio indicating some degree of inclination, although it is nearly face-on. The central bulge region appears to have a high concentration of stars. There seems to be a slight asymmetry in the outer disk, potentially due to tidal interactions or past minor mergers.