This galaxy presents a lenticular morphology, exhibiting a prominent central bulge and a flattened disk. The bulge appears smooth, with a concentrated luminosity profile. The disk, while visible, lacks distinct spiral arm structure. The overall color of the galaxy suggests an older stellar population, with relatively little ongoing star formation.

The galaxy exhibits a slight asymmetry in its shape, hinting at a possible past interaction or minor disturbance event. A faint tidal tail seems to stretch out, further suggesting this. The galaxy appears relatively isolated, without any immediate companions.
