The galaxy presents as a spiral type, exhibiting a disk-like structure with prominent spiral arms. These arms emanate from a central bulge region, which is moderately sized relative to the disk. The arms are primarily defined by their medium winding, tracing a relatively open morphology as they extend outward. There appear to be two dominant spiral arms. There is no evidence of tidal tails or significant morphological distortions, indicating no major interaction. Star formation appears to be taking place within the spiral arms. A bar is visible, but it seems to be weak. The color index suggests a general population of intermediate-age stars, with bluer hues concentrated along the spiral arms indicating regions of ongoing star formation. The galaxy is not observed edge-on.
