The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. It exhibits a spheroidal shape, appearing mostly round, with minimal visual evidence of spiral arms or a distinct disk structure. The light distribution suggests an older stellar population, as indicated by the yellowish-red hue, with a likely low rate of ongoing star formation. There's no obvious indication of recent or ongoing merger activity, and no noticeable tidal features or asymmetries are apparent in its structure. The galaxy appears to be relatively isolated in its immediate vicinity. Its apparent size is small, suggesting it is at a considerable distance.
