The galaxy appears to be a spiral galaxy, presenting a near face-on orientation relative to our line of sight. The central bulge exhibits a high degree of smoothness and is slightly elongated. Surrounding the bulge, a disk is visible, showing evidence of spiral arm structure. The spiral arms are relatively tightly wound. The galaxy is dominated by a central bulge and appears to have a single or double spiral arm structure. The galaxy does not show any signs of recent merging activity. There are no major disturbances or tidal tails. The overall color suggests a mixed stellar population, with some regions of active star formation, as indicated by the faint blue coloring. The overall morphology indicates that it is a relatively undisturbed spiral galaxy.
