The galaxy presents a generally smooth morphology, exhibiting a high degree of central concentration. The light profile appears elliptical, approaching a circular shape. There is a lack of significant dust lanes, spiral arms, or bar structures visible. A slight color gradient is noted, with the central region appearing more yellow than the outer edges, suggesting an older stellar population centrally located. Overall, there does not appear to be any evidence of significant disturbances to the structure. The light is highly concentrated and the galaxy has a magnitude that would suggest this is a very large, relatively bright galaxy. There may be some very slight distortions or disturbances, however the galaxy is overwhelmingly appearing to be undisturbed. 
