The galaxy presents a morphology suggestive of an elliptical type, exhibiting a smooth, somewhat rounded light distribution. The concentration of light is highest towards the center, with a gradual decrease in intensity towards the outer regions. There may be a subtle disk-like feature. The color appears generally yellow/orange, possibly indicative of an older stellar population with reduced star formation activity. There are some indications of a potential minor disturbance. The overall structure appears relatively undisturbed, however.
