This galaxy presents as a disk-shaped system viewed at a significant inclination. The central bulge is moderately prominent, exhibiting a smooth, elliptical morphology. A faint, disk component extends outwards from the bulge. The disk appears relatively featureless. There is evidence of some internal color variation within the galaxy, with a slightly redder hue concentrated in the central region, potentially indicating a higher density of older stellar populations. The outer regions of the disk appear slightly bluer, possibly indicating more recent star formation. The galaxy does not appear to be undergoing any major merging events or significant tidal interactions, with a generally undisturbed structure. It is likely a relatively massive galaxy with a moderate rate of star formation.
