This galaxy presents as a relatively smooth, elliptical-like structure. The central region is bright and concentrated, exhibiting a yellowish-green hue suggesting a population of older stars. Fainter, diffuse light extends outwards from the core, and the overall form is generally rounded. There is a hint of asymmetry or a minor disturbance visible on the upper side, possibly indicative of a past or ongoing interaction, although no major disruption to the overall structure is immediately apparent. The colour gradient suggests a possible decline in star formation activity from the center outwards.
