This galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated, bright, yellowish-orange hue. Fainter, diffuse bluish-green light surrounds the central region, extending outwards in a somewhat spherical shape. No distinct spiral arm structures or dust lanes are readily apparent. The galaxy appears to be isolated, showing no signs of major tidal disturbances or ongoing mergers with other galaxies. The overall morphology suggests a system dominated by an older stellar population, with a lower rate of ongoing star formation within the extended halo.