The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the color gradually shifts towards a reddish-orange, potentially indicating the presence of dust or a population of evolved stars. The outer regions of the galaxy are more diffuse and less well-defined, with a subtle elongation apparent, departing slightly from a perfectly circular morphology. There's no obvious evidence of a spiral arm structure or strong tidal features indicative of a recent major merger event; however, there are some hints of minor disturbances in the evenness of the light distribution. The overall light profile suggests a system dominated by bulge-like features, with potentially low levels of ongoing star formation activity.
