The galaxy presents a morphology dominated by a smooth, centrally concentrated component. It exhibits an elliptical shape, with the ratio of the major to minor axes indicating a modest degree of flattening. The central region displays a high surface brightness, suggesting a significant concentration of stars and possibly a supermassive black hole at the core.

A faint, extended disk is perceptible surrounding the central bulge. There is a faint blue structure near the galaxy, which may indicate star formation occurring. The overall color of the galaxy appears relatively red, hinting at an older stellar population with a diminished rate of star formation, though blue light near the galaxy could indicate otherwise. Faint tidal features suggest recent or ongoing gravitational interactions. The galaxy exhibits an estimated effective radius of a few kiloparsecs.
