The galaxy presents a generally smooth morphology with a hint of internal structure. It appears to be composed of a brighter central region with slightly diffuse, fainter extensions. The core exhibits an elliptical shape, and a moderately elongated, cigar-like structure.

A degree of asymmetry is observable within the galaxy's structure, with the light distribution more concentrated towards one end. This suggests a recent or ongoing interaction or merger event, as indicated by a possible minor disturbance. The overall color is indicative of an older stellar population, with a discernible reddening compared to younger, bluer galaxies, implying a relatively low specific star formation rate.
