The galaxy appears to be a single, relatively smooth object, displaying a moderate level of roundness. There is no discernible spiral structure or a prominent disk. The galaxy exhibits a yellowish-white hue in the central region, which fades into a blueish-white at the edges. This may imply a generally older stellar population within the central bulge, with ongoing, but moderate, star formation occurring in the outer regions. There is a slight asymmetry in the galaxy's shape, possibly indicating minor gravitational interaction with another galaxy, though no clear signs of a major merger event are present. Overall, the galaxy seems to be a generally undisturbed system, with a likely elliptical or lenticular morphology.
