The galaxy presents as a relatively small, lenticular or early-type spiral structure. Its central bulge is prominent, displaying a smooth, concentrated light profile. There is a subtle indication of a disk component surrounding the bulge, however it is difficult to determine defined spiral arm structure. The disk appears relatively homogenous in color. The galaxy's overall shape is somewhat elongated, but generally close to round. There are no obvious signs of major interactions or mergers, however, there is a slight visual irregularity that could suggest a minor disturbance. The galaxy exhibits a color profile indicative of an older stellar population, with a subtle shift towards redder wavelengths. There is little evidence of significant ongoing star formation within the galaxy.
