The galaxy presents as a slightly elongated, cigar-shaped structure. Its light profile appears smooth and relatively featureless. A bright central bulge dominates the morphology, with the luminosity decreasing gradually towards the outer edges. There is some visual suggestion of a disk, but it is not well defined. The galaxy exhibits a subtle color gradient; the central region shows a yellowish-white hue, transitioning to a bluer tint towards the periphery. This color distribution may indicate a varying stellar population, with older stars concentrated in the center and younger stars in the outer regions, potentially associated with ongoing or recent star formation. There are hints of minor structural disturbances or asymmetries, possibly indicating past interactions or minor merger events.
