The galaxy presents as a relatively small, compact object. The color profile suggests a stronger emission in the green and blue wavelengths, indicative of potentially younger stellar populations or active star formation. The overall morphology appears somewhat disturbed, with a possible faint disk-like structure or tidal feature oriented approximately horizontally across the main body of the galaxy. This feature could indicate a minor gravitational interaction or recent merger event. The galaxy lacks a clear central bulge, giving it a flattened appearance. There is no spiral arm structure immediately discernable. The object does not display a high level of smoothness.
