The galaxy presents as an elliptical-like structure, moderately elongated along its major axis. Its color profile suggests a dominant population of older stars, evidenced by the reddish-yellow hue concentrated in the central bulge. Fainter, greenish diffuse light extends outward from the core, possibly indicating the presence of some younger stars or active star-forming regions. The galaxy appears relatively smooth in texture with no prominent spiral arm structures visible. Based on the disturbance estimates, the galaxy has some indications of a possible past or ongoing minor disturbance.
