The galaxy presents a generally smooth morphology. The primary structure appears as a moderate-sized elliptical shape, exhibiting a concentrated central bulge that fades into the outer regions. Color gradients suggest an older stellar population, showing predominantly yellowish hues that are consistent with less active star formation. There appears to be a potential merging event underway, with a second, smaller mass located at a small distance from the primary mass. Evidenced by some possible disturbances in the main galaxy's morphology. Given the smoothness and color, the system could be classified as an early-type, possibly undergoing interactions with other galaxies.

