The galaxy presents as an amorphous structure with an irregular morphology. There is a lack of clear spiral arms or a defined elliptical shape. The light distribution appears diffuse and mottled. The galaxy exhibits a clumpy appearance with several bright, knot-like regions, possibly indicative of active star formation. There is little evidence of a prominent central bulge. The color distribution is uneven, with blue-shifted areas suggesting younger stellar populations and/or less dust attenuation, and redder areas hinting at older stellar populations or higher dust content. There appears to be some distortion in the galaxy's overall shape, possibly due to tidal interactions or internal processes.
