The galaxy presents a primarily smooth morphology, with a slight elongation suggestive of a disk-like structure. The central bulge exhibits a yellowish-white hue, potentially indicative of an older stellar population. Surrounding the bulge, faint, irregular features are visible. These features display a bluer tint, which may be indicative of ongoing star formation. There is a subtle asymmetry to the overall structure, but no strong evidence of a major merger event is directly apparent in the image. It is observed at redshift z=0.108184.