The galaxy presents as a lenticular or possibly spiral type, seen at an oblique angle relative to our line of sight. The central bulge appears relatively prominent and elongated, displaying a yellowish-white hue, suggesting an older stellar population. There's an indication of a disk structure extending outwards from the bulge, exhibiting a bluer tint, perhaps indicating ongoing star formation or a younger population of stars. Faint hints of spiral arm structure are suspected, albeit poorly defined. The overall morphology appears to be mostly undisturbed, with no clear signs of major merger activity. The galaxy presents a smooth appearance, with some subtle features suggesting the presence of a disk component.
