The galaxy presents a largely smooth morphology, appearing elliptical in shape. The light profile shows a concentrated central bulge that emits strongly in the green and red bands, suggesting an older stellar population. There is a faint, diffuse halo surrounding the bulge that emits in the blue and green bands. No distinct spiral arms or prominent dust lanes are discernible. The overall color suggests a relatively quiescent system, with little ongoing star formation, though hints of blue emissions suggest that it is not entirely quiescent. There may be minor tidal disturbances in the galaxy.
