The galaxy presents a generally smooth morphology, with a dominant central bulge. The bulge appears nearly spherical. A faint disk appears to surround the central bulge, and is roughly twice the diameter of the bulge. Hints of a spiral structure are present within the disk, but are not very well defined. The galaxy's color suggests a mix of stellar populations, with a slightly higher concentration of older stars in the central bulge. A few bluer regions are apparent within the disk, potentially indicating areas of ongoing star formation. There is some indication of minor disturbances or irregularities in the galaxy's outer regions, possibly due to tidal interactions or minor mergers, but no major merging events are easily visible.
