The galaxy presents as a single, diffuse object with a relatively smooth overall texture. Its morphology appears elliptical or spheroidal, lacking any distinct spiral arm structures or a prominent disk. The light distribution is centrally concentrated, with a bright core that gradually fades towards the outer regions. The color profile suggests an older stellar population, as it leans towards redder wavelengths. No signs of ongoing major mergers or tidal disturbances are readily apparent in the image. Minor irregularities or faint features may be present upon closer inspection, however, the overall impression is that of a relaxed system.
