The galaxy presents as a slightly elongated, lenticular structure. The central region exhibits a bright, concentrated bulge, appearing yellowish-white, indicative of an older stellar population. Surrounding this bulge is a fainter, more diffuse disk. The disk appears relatively smooth with hints of spiral arm structure. The color of the disk is a muted blue, suggesting the presence of some ongoing star formation, although the rate appears to be quite low. There is a slight asymmetry in the overall shape, possibly indicative of a minor gravitational interaction or disturbance. The galaxy's structure is largely dominated by the smooth central bulge, with a significant fraction of the light emanating from this region. There may be some tidal features or faint extensions visible on the periphery, however they are faint. The galaxy is approximately 5 kpc across.
