The galaxy appears to be a spiral type, with a central bulge and a disk component. The bulge exhibits a yellowish hue, suggestive of an older stellar population, potentially with a lower rate of on-going star formation compared to other regions of the galaxy. The disk shows a bluer color, hinting at the presence of younger, hotter stars. The spiral arms seem to be moderately tightly wound. A bar-like structure appears present across the center of the galaxy, with some evidence for defined spiral arms originating from near the ends of the bar. The size of the bulge relative to the overall galaxy appears moderate. No large-scale tidal disturbances or major merger features are readily apparent. The galaxy seems to be relatively undisturbed, with only a slight chance of minor disturbance.
