The galaxy exhibits a distinct spiral structure, characterized by tightly wound arms emanating from a central bulge. The bulge appears moderately prominent and exhibits a yellowish hue, indicative of an older stellar population. The spiral arms themselves display a bluer color, suggesting active star formation regions.  The galaxy appears relatively undisturbed, with no obvious signs of a major merger event. The overall shape appears elliptical, but nearly circular, and the arms are discernible but not strongly defined. The central region shows a higher concentration of light.
