The galaxy presents a generally smooth, elliptical morphology. Its overall shape appears to be somewhere between round and oblong. There is little evidence of spiral arms or distinct features typically associated with disk galaxies. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges. The galaxy exhibits a yellowish hue, potentially indicating an older stellar population with reduced current star formation. There appears to be a possible merger or significant interaction occurring with the central galaxy, creating a disturbed morphology and a faint extension, but it is difficult to see due to its distance.
