The galaxy presents as a somewhat smooth, disk-like structure. It exhibits an overall elliptical shape, appearing more elongated than perfectly circular. A central bulge is subtly visible, though not highly pronounced. Color gradients are present, with the core region displaying a slightly yellower hue, possibly indicating an older stellar population. Some indications of minor disturbances are present, suggesting the possibility of ongoing or recent interactions with another galaxy. Possible merger remnant, or tidal distortions are present. The galaxy's profile is not entirely uniform, showing hints of internal structure, but lacking distinct spiral arms.
