The galaxy presents as a relatively compact object with a disk-like structure. The central region exhibits a bright, concentrated bulge, appearing somewhat yellow-white. This suggests an older stellar population dominating the core. Surrounding the bulge, there's a distinct, though not sharply defined, disk component. This disk shows hints of spiral arm structure, but it's not well-resolved. The disk displays a subtle blue hue, hinting at the presence of younger, hotter stars and ongoing star formation, though not at a particularly high rate.

A faint, extended halo of diffuse light surrounds the galaxy, indicating the presence of a stellar halo, possibly mixed with some dust and gas. The overall smoothness of the galaxy suggests a well-evolved system without significant ongoing major mergers, although minor disturbances can not be excluded.
