The galaxy presents a generally smooth morphology, with a largely featureless disk. It appears relatively round in shape, deviating only slightly from perfect circularity. There is some visual evidence of possible disturbances in the galaxy's structure, which could be indicative of minor gravitational interactions. Faint wisps surround the object, possibly indicative of tidal interactions. The galaxy exhibits color gradients, with the central regions appearing more yellow, potentially suggesting an older stellar population. The outer regions show hints of bluer hues, implying the presence of younger stars. The overall appearance of the galaxy suggests an evolved system, potentially undergoing interactions with other galaxies or a recent merger event.
