The galaxy presents as a single, largely smooth structure with a high degree of central concentration. It exhibits an elliptical morphology, deviating slightly from a perfect circular shape towards a more elongated, cigar-like form. The core region displays a yellowish-orange hue, suggestive of an older stellar population. Surrounding the central region, the galaxy gradually transitions to a slightly bluer tint, which may indicate the presence of some younger stars. Faint traces of a disk-like structure can be inferred, though the overall appearance is dominated by a smooth, featureless light distribution with no apparent spiral arm structures or significant dust lanes. There is no strong evidence of recent or ongoing major merger activity.
