The galaxy appears as a slightly elongated structure with a noticeable central bulge. The light distribution suggests a disk galaxy, although details are somewhat obscured. The color gradient indicates older stellar populations concentrated towards the center, showing a yellowish hue. The outer regions of the galaxy appear fainter, with hints of bluer light, potentially indicating regions of recent star formation. The overall structure exhibits a relatively smooth profile, with no obvious signs of strong disturbances or major interactions. A slight tilt relative to our line of sight is evident from its elliptical appearance. 
