The galaxy presents as a spiral with a moderately sized central bulge. The spiral arms are well-defined, exhibiting a relatively tight winding pattern. Two primary spiral arms are clearly visible, though determining the exact arm count is somewhat challenging due to the image resolution and arm complexity. There is no obvious bar structure. Evidence suggests some minor gravitational disturbance. The overall color profile indicates a mix of stellar populations, with a yellower hue in the central bulge potentially indicating older stars and a bluer tinge in the spiral arms indicating ongoing star formation. The galaxy is not observed edge-on.
