The galaxy presents as a slightly elongated, relatively bright object. It exhibits a prominent central bulge, which appears yellowish-white, suggesting an older stellar population. Fainter, bluish spiral arms extend from the bulge, with the overall structure appearing somewhat diffuse and flocculent. The galaxy appears to be at a moderate angle relative to our line of sight. There's no strong evidence of significant tidal disturbances or ongoing major mergers, although subtle asymmetries or minor disturbances cannot be ruled out at this resolution.
