The galaxy presents as a somewhat symmetrical, centrally concentrated object with a generally smooth appearance. There is a slight elongation, suggesting a deviation from a perfectly spherical shape, trending towards a more elliptical morphology. The primary light source appears to emanate from the central region, with a gradual decrease in intensity moving outwards. There is subtle color variation across the galaxy; a slight blueish tint is visible in the outer regions and a yellow/redish hue at the center. This suggests a slightly older stellar population is more concentrated toward the center, with perhaps some ongoing or recent star formation present in the disk. Faint irregularities in the outer regions hint at possible minor gravitational interactions. Overall, the galaxy seems to be relatively evolved and massive.
