The galaxy presents as a smooth, centrally concentrated elliptical-like morphology. There is a high likelihood of a smooth structure, with a notable lack of spiral arms or defined disk-like features, though there is a very low possibility of a minor disturbance. The overall shape can be described as in between round and cigar shaped. The galaxy exhibits a significant reddish hue, indicative of an older stellar population and reduced recent star formation activity. Based on this color, the galaxy is likely a massive system.