The observed galaxy presents as a flattened, disk-like structure, seen at an oblique angle relative to our line of sight. The central region exhibits a bright, concentrated luminosity, suggestive of a prominent galactic nucleus or bulge. Surrounding this core, a less intense, more diffuse region is visible, likely indicating the presence of a galactic disk. The outer edges of this disk appear somewhat irregular. The color profile across the galaxy reveals a gradient, with the central bulge exhibiting a bluer hue compared to the more reddish outer regions. The overall structure does not present any obvious signs of ongoing major merger activity, though some subtle irregularities in the disk shape could imply minor disturbances, or potential minor merging. The smoothness of the light distribution varies, with the central bulge appearing smoother and the outer disk showing more granular texture. The galaxy shows a slight ellipticity, giving it an oval shape, which further suggest an inclination angle.
