The galaxy displays a clear disk morphology and appears to be oriented at an angle relative to our line of sight. The color gradients suggest a stellar population that is more centrally concentrated, potentially indicative of a bulge. Faint arms are visible, characterized by a relatively open, grand design spiral structure. The presence of bright blue regions are concentrated with the arms, suggesting sites of recent or ongoing star formation. There may be a slight bar feature present in the central region, although its prominence is not clear. No major mergers appear to be in progress, but there may be subtle tidal features present hinting at minor interactions in the past.