The galaxy presents as a relatively well-defined, though somewhat diffuse, structure. The central region exhibits a concentrated luminosity with a yellow-orange hue, possibly indicative of an older stellar population. Surrounding this core is a bluer, less concentrated region that appears to extend outwards, hinting at the presence of a disk. There are subtle asymmetries in the outer regions. These features suggest that the galaxy is not entirely featureless and may be undergoing some form of interaction or disturbance, even potentially a minor merger event.
