The galaxy presents as a spiral, exhibiting a distinct disk structure. Two prominent spiral arms are clearly visible, tracing a path outward from the central bulge. The bulge appears moderately sized and bright, with a concentrated luminosity suggesting a significant stellar population. A bar structure is suspected along the galaxy's core, indicated by a slightly elongated central region. The winding of the spiral arms appear medium and somewhat patchy. There is no clear evidence of ongoing major merging activity, and the disk appears relatively undisturbed.
