The galaxy presents as a primarily smooth structure with a slight elongation, appearing somewhere between round and cigar-shaped. It exhibits a central concentration of light, suggesting a bulge component. Faint, diffuse features extend outwards from this core, implying the presence of a disk. The color profile transitions from a yellowish-white core to redder hues in the outer regions. There are no apparent major disturbances or indications of ongoing merging events in this image, though some minor disturbances can be seen in the faint, outer regions.
