The galaxy presents as a moderately inclined spiral or disk galaxy. There is a clear central bulge that appears quite smooth, and possibly contains older stars. Fainter spiral arms extend from the bulge, appearing somewhat flocculent and less well-defined. These arms show a bluer tint than the core, indicating the presence of younger, hotter stars and star formation regions. The overall color of the galaxy appears to be in the yellow-green range, suggestive of a mix of stellar populations. There is some indication of a slight warp or disturbance in the outer disk, although this could be due to limitations in image resolution. No obvious signs of a major merger are immediately apparent.