The observed galaxy presents a moderately inclined, somewhat elongated morphology. Its overall color profile appears generally blue, indicating the presence of a younger stellar population and ongoing star formation. While a distinct spiral structure is not readily apparent, there may be some subtle evidence of disk features. The light distribution is relatively smooth, however there is some indication of possible slight disturbances or minor irregularities in its structure suggesting interaction with other galaxies. It possesses a stellar mass on the smaller end, and has a relatively low star formation rate. The galaxy appears intermediate in shape between round and elongated. Overall, the galaxy appears to be an actively star forming dwarf galaxy. 
