The galaxy presents as a moderately luminous, early-type spiral, potentially an Sa or Sb classification. It exhibits a prominent, bright central bulge that dominates the overall luminosity profile. The color of the bulge is yellowish-white, suggesting an older stellar population with limited ongoing star formation. Fainter, bluish-white regions are observed surrounding the central bulge, indicative of some younger stars and regions of active star formation within the galactic disk.

The galaxy appears moderately inclined to our line of sight, revealing a flattened disk structure. There is no evidence of strong tidal interactions or major mergers. There is a possibility of a weak bar structure. Overall, the galaxy presents a relatively smooth appearance, with a subtle disk that fades into the background sky.
