The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the visual structure. The bulge appears to be surrounded by a fainter, more diffuse halo of stellar material. There is little evidence of distinct spiral arm structure or prominent dust lanes. The galaxy appears to be relatively undisturbed, with no obvious signs of recent or ongoing major merger activity, although there may be some minor disturbance in the outer regions. The color profile suggests a population of older stars, particularly concentrated in the central bulge, with a slightly bluer component present in the outer regions. The overall shape tends toward roundness, but it has a slight elongation.