The galaxy appears to be a relatively smooth, elliptical-like object with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population of older stars and a lower rate of ongoing star formation. There is some evidence of a slight asymmetry or minor disturbance in its morphology, although the overall structure appears largely undisturbed. The galaxy is generally round in shape, with the possibility of a faint and diffuse halo surrounding the brighter central region.
