The galaxy presents a distinct disk-like morphology, viewed at a significant inclination. Its overall structure suggests an elliptical shape, with the major axis noticeably longer than the minor axis. A prominent central bulge is visible, exhibiting a yellowish hue, which could indicate an older stellar population dominating this region. Surrounding the bulge, there is a fainter, bluer disk component. While spiral arms are not clearly resolved, the uneven distribution of light within the disk may suggest the presence of underlying spiral structure. There appear to be no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy's color gradient, transitioning from yellowish in the center to bluer in the outer regions, could signify radial variations in stellar populations, with younger, bluer stars populating the disk and older, redder stars concentrated in the bulge.
