The galaxy presents as a primarily smooth, elliptical-like structure with a high degree of central concentration. The galaxy exhibits a yellowish-orange color, which could indicate an older stellar population. The overall shape appears to be moderately elliptical, tending towards a rounded form but not perfectly circular. There is no evidence of strong spiral arm structures or prominent dust lanes visible in the image. Faint irregularities and disturbances at the edge of the galaxy may indicate a minor interaction or ongoing merger.
