The galaxy presents a somewhat ambiguous morphology. The central region appears bright and relatively smooth, possibly indicating an older stellar population or a bulge component. Fainter, diffuse structures surround the central region, hinting at a possible disk or spiral arm features. However, these features are not well-defined, leading to an appearance of irregularity. A notable elongation is visible, suggesting a non-spherical shape, somewhere between round and cigar shaped. There might be a minor interaction or disturbance in the galaxy's structure, although the features are not clear enough to confirm a major merger event. Overall, this galaxy appears to be a low-mass system, with modest star formation activity.
