The galaxy presents a flattened, elongated morphology, strongly suggesting a disk-like structure observed at a high inclination angle. It is oriented approximately along the north-west to south-east axis. The light distribution appears centrally concentrated, with a brighter, more compact central region. This central region exhibits a distinct bluish hue, potentially indicative of recent or ongoing star formation activity. The outer regions of the disk fade gradually into the background, showing a smoother texture and a slightly redder coloration. There is a subtle asymmetry along the major axis, with one side appearing more extended and diffuse than the other. There is no clear evidence of spiral arm structure, or any kind of disturbance/merging going on.
