The galaxy presents as a moderately inclined spiral system. There is a notable central bulge with a yellowish hue, indicative of an older stellar population. Fainter, bluer spiral arms extend from this central region. These arms suggest ongoing star formation. The galaxy's disk appears relatively thin. The overall light distribution suggests that the galaxy is not perfectly symmetric, possibly due to gravitational interactions. The galaxy's morphology suggests a low Sersic index, generally consistent with spiral galaxies. The system's radial light profile is generally smooth, although some features may exist in the outer regions.
