The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central region that gradually fades into the outer edges, lacking prominent spiral arm structures or a distinct disk. The morphology suggests a spheroidal shape, with a high degree of roundness. There appears to be little to no major disturbance in the overall structure, such as tidal tails, indicating it is not currently undergoing a major merger event. However, there may be minor irregularities in its shape which hint at potential past gravitational interactions. There is no evidence of a very active star formation. The light is subtly redder than the light of other field galaxies. This indicates an older stellar population as well as an apparent redshift.
