The galaxy presents as a relatively compact, disk-like structure with a noticeable central bulge. The overall color profile suggests a predominantly older stellar population, evidenced by the reddish hue observed in the disk. A slight bluer component is visible in the central region, which may indicate some ongoing star formation, albeit at a seemingly low rate.

The disk appears relatively smooth, with no prominent spiral arm structures discernible in the image. There is a faint hint of a possible dust lane along the plane of the disk, indicating the presence of interstellar matter within the galaxy. However, the overall appearance is primarily smooth and undisturbed. The lack of significant tidal features or distortions suggests that the galaxy has not experienced a recent major merger event. Minor disturbances may be present, but are not immediately evident at this resolution. The observed morphology aligns with that of a relatively undisturbed spiral or lenticular galaxy.
