The galaxy appears as a centrally concentrated, elliptical structure with a smooth, diffuse light profile. There is a distinct lack of spiral arms or prominent dust lanes. The core exhibits a bright, golden hue, suggesting a high concentration of older stars. The galaxy's overall color gradient transitions smoothly from the yellowish center to a slightly redder periphery. The overall shape is nearly circular, with only a very slight deviation from perfect roundness. There is no visible evidence of any ongoing major merging events or significant tidal distortions in the outer regions. Indications of minor disturbances may be present, but are not readily observable. Star formation activity appears subdued.
