The galaxy presents as a centrally concentrated system with a smooth, diffuse light profile. It exhibits a nearly circular morphology, with a slight deviation towards a more intermediate elliptical shape. The galaxy's color profile appears relatively homogeneous, dominated by a yellowish hue, potentially indicative of an older stellar population. There is a slight suggestion of an interaction or merger event occurring, given a potential minor disturbance in the galaxy's outer isophotes or perhaps even a secondary nucleus. The overall appearance favors a mature system with a high degree of central symmetry. Limited evidence suggests active star formation, but I would need additional multiwavelength data to verify this.
