The galaxy presents as a relatively small, moderately bright object. Its morphology appears disturbed. There is some indication of spiral structure, particularly one arm appearing more distinct than the others. This arm seems elongated and slightly warped.

The galaxy's color profile suggests active star formation, with regions of bluer light. The central region of the galaxy displays a more concentrated distribution of light, possibly indicating an older stellar population or a bulge. There are some irregular color variations in the central core, possibly indicating some kind of distortion.

Overall, the galaxy exhibits features characteristic of a system undergoing some gravitational interaction or possessing internal irregularities. There is evidence of ongoing star formation, and possible evidence of disturbed morphology, likely from a merger or other gravitational interaction.
