This galaxy presents as a single, largely featureless entity. The light profile suggests a spheroidal morphology, with a high degree of central concentration. A smooth and homogenous light distribution dominates, diminishing outwards from the core with no readily apparent spiral arms or bar structures. The color gradients indicate a population of older stars towards the center, trending towards a redder hue, and a slight blue component present towards the outer regions, potentially indicative of some ongoing, but likely low level, star formation. The lack of substantial dust lanes or other disruptive features suggests minimal recent merging activity, though some slight asymmetry in the outer halo may be evidence of minor gravitational interactions. Given the overall smooth appearance and color profile, this galaxy likely possesses a significant stellar mass.
