The galaxy presents as a central, concentrated bulge of older stars exhibiting a reddish-yellow hue. Surrounding this core is a more diffuse disk component, showing a bluer tint suggesting regions of more active star formation. There appear to be some asymmetrical features or disturbances in the outer regions of the disk, possibly indicative of tidal interactions or past minor mergers. A small proportion of the galaxy appears smooth, while the majority seems to show evidence of disk-like structures or more complex features. The system does not appear to be completely isolated, implying gravitational interactions may be ongoing.