The galaxy appears to be a lenticular or early-type spiral system, displaying a prominent bulge and a faint, diffuse disk. The bulge exhibits a yellowish-white color, suggesting an older stellar population, while the disk shows bluer hues, indicative of more recent star formation. The galaxy's overall shape is elliptical with a high degree of roundness, but hints of a flattened disk-like structure are visible. No strong spiral arm structure or bar feature is readily apparent. There is minor indication of a possible gravitational disturbance or interaction, although no definitive merger features are discernible. The galaxy's light profile appears smooth and centrally concentrated, with a gradual decrease in surface brightness away from the core.
