The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge with a noticeable radial decrease in luminosity outward. The overall color is yellowish, suggesting a population of older stars. There is little evidence of distinct spiral arms or significant dust lanes. The morphology suggests an early-type galaxy, possibly an elliptical or lenticular, with a high degree of central concentration. No obvious signs of ongoing major mergers or tidal disturbances are visible. Based on its relatively high level of smoothness, it does not exhibit much star formation.
