The galaxy presents a generally elliptical morphology. Its structure appears largely featureless, with no immediately obvious spiral arms or significant dust lanes. A bright, concentrated central bulge dominates the light profile. The color is generally red-shifted with a yellow-orange hue, suggesting a population of older stars with limited ongoing star formation. The galaxy exhibits a high degree of symmetry and no immediately apparent signs of tidal disturbances or interactions. The outer regions fade gradually into the background, without abrupt cutoffs or shell-like structures.
