The galaxy appears as a relatively compact, somewhat diffuse object. It exhibits a smooth overall morphology, with little evidence of defined spiral arms or a prominent central bulge. There may be a slight flattening of the galaxy's shape, moving it away from a perfect circle. The color profile suggests a mix of stellar populations, with some regions appearing slightly redder than others. This could indicate a varying distribution of older, cooler stars and younger, hotter stars within the galaxy. There seems to be some minor disturbances, which could be attributed to past minor interactions. There is no clear evidence of a major ongoing merger or significant tidal distortions in its overall structure.
