The galaxy presents as a relatively smooth, elliptical-like object with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting a substantial population of older stars. Fainter, somewhat bluish-white light surrounds the core, extending outwards in a diffuse halo. The overall shape indicates that it is neither perfectly spherical nor highly elongated, and I do not detect any prominent spiral arms or a well-defined disk structure. There is no readily apparent evidence of ongoing major merging events or significant tidal disturbances, though there may be some minor irregularities in the outer regions, which indicates minor disturbances. It shows an intermediate roundness, and there is very little cigar shape. The galaxy seems to be a relatively quiescent system.
