The galaxy presents with a dominant central bulge, exhibiting a yellowish-white hue indicative of an older stellar population. The bulge appears relatively smooth, with limited apparent substructure. Surrounding the bulge, there's a fainter, bluer disk component. The bluer color suggests regions of more active star formation within the disk. The overall shape of the galaxy appears somewhat irregular, hinting at possible gravitational interactions or recent merger activity. There is a slight extension visible on one side, which might indicate tidal features. Despite the presence of a disk, the galaxy lacks a well-defined spiral structure. The galaxy appears to be relatively compact.
