The galaxy presents as a largely smooth, elliptical-like structure, exhibiting a concentrated central bulge. There is a general lack of defined spiral arms or distinct features typically associated with disk galaxies. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region and a slight reddening towards the outer edges. The overall light distribution is relatively uniform, with no apparent signs of recent major mergers or significant tidal disturbances. The galaxy appears moderately compact with a high degree of symmetry, suggesting a dynamically relaxed system.
