This galaxy presents a prominent, relatively well-defined disk structure when viewed from our current perspective. The central bulge appears compact and exhibits a yellowish-white hue, potentially indicating an older stellar population within the core region. The disk itself displays a multi-colored appearance, with an inner region showing a brighter blue-white coloration. The outer edges of the disk show hints of redder hues that are concentrated in rings, likely due to dust obscuring the underlying star formation or potentially indicating regions of ongoing star formation within dustier environments.

Some faint, diffuse light extends outwards from the main disk, creating a somewhat irregular halo-like structure. The overall shape is more akin to a relatively circular and defined structure compared to an irregular form. Possible signs of tidal disturbances are observed, these features seem minor, but they could point towards recent or ongoing gravitational interactions with other galaxies. These disturbances may be responsible for some of the irregularity observed in the outer halo.
