The galaxy presents a generally smooth, elliptical morphology. Its overall shape is relatively round, with a concentrated central bulge that emits light primarily in the yellow spectrum. The outer regions of the galaxy exhibit a broader halo, with a mixed color profile including hints of blue, which might suggest on-going star formation. However, the smoothness of the profile suggests that this galaxy could be transitioning to passive evolution. Evidence of gravitational disturbance, merging or tidal tails is weakly apparent.
