The galaxy presents as a relatively compact object with a smooth overall appearance. Its shape is somewhere between a perfect circle and a more elongated form. A slight asymmetry is observed in its light distribution, suggesting a deviation from a perfectly uniform ellipsoid. There is no strong evidence of spiral arm structures, bar features, or a prominent central bulge. The galaxy appears to be relatively isolated, without any obvious signs of major interactions or mergers. The overall color is somewhat reddish, implying a potentially older stellar population, as opposed to one dominated by young, blue stars associated with vigorous star formation. There's a very slight hint of a possible minor disturbance on one side, though more data would be needed to confirm if this is intrinsic to the galaxy or a result of imaging artifacts.
