The galaxy presents a generally smooth morphology, with no immediately obvious spiral arm structure. The galaxy appears disk-shaped and is viewed at a moderate inclination, presenting an elliptical profile. A central bulge is present, appearing concentrated and relatively bright. The bulge region is surrounded by a less luminous, more diffuse disk component. There appears to be a subtle color gradient within the galaxy, with the central region exhibiting a somewhat redder hue compared to the outer regions of the disk, which are bluer in colour. The outer regions of the disk fade gradually, indicating a relatively smooth decline in stellar density with increasing radius. Overall, the galaxy exhibits characteristics of a typical disk galaxy with a noticeable bulge.
