The galaxy presents a generally smooth appearance, with a dominant central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. A faint, diffuse disk appears to surround the bulge. Within the disk, hints of spiral structure may exist, but the image resolution limits definitive characterization. There is a slight hint of bluer regions within the disk, but these regions are not very prominent, suggesting moderate star formation activity. The galaxy has an overall elliptical shape and does not show any indications of major mergers or significant tidal disturbances. The roundness is in between that of round and cigar-shaped galaxies.
