The galaxy appears to be a relatively smooth, elliptical-like system at a considerable distance. The light is concentrated towards the center, suggesting a high degree of central mass concentration. The overall color of the galaxy is relatively red, indicative of an older stellar population and potentially lower levels of ongoing star formation. There is some evidence of possible tidal distortions in the outskirts, indicating it may be in the process of merging.

It exhibits a round shape and is generally smooth in appearance, with a small percentage of the light in the disk. The galaxy's size is moderately large. Its red color indicates the presence of older stars and a low star formation rate, with only a few regions showing signs of any star formation.
