The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellowish hue, possibly indicating an older stellar population within the core. Fainter, bluer light surrounds this central region, suggesting the presence of some younger stars or ongoing star formation, although at a low rate. The galaxy lacks any distinct spiral arms or a prominent disk. Its overall shape is generally round, with no significant signs of tidal disturbances or ongoing mergers.
