This galaxy presents as a relatively elongated, likely spiral, system viewed nearly edge-on. A bulge is visible, appearing somewhat centrally concentrated and exhibits a yellowish hue, suggesting an older stellar population. The disk component extending from the bulge displays a bluer tint, indicative of ongoing star formation. The disk seems relatively smooth in appearance, with little evidence of strong spiral arm structures or prominent dust lanes discernible at this resolution. The galaxy's overall morphology hints towards an Sa or Sb classification. The system appears isolated, with no obvious signs of major tidal interactions or mergers.
