The galaxy presents as a relatively smooth, centrally concentrated object, indicative of an elliptical morphology. Its overall shape is neither perfectly spherical nor highly elongated, leaning more towards an intermediate elliptical form. There is little evidence of spiral arms or a prominent disk structure. The light distribution suggests a lack of significant ongoing star formation within the galaxy's core. There is a slight asymmetry in the galaxy's outer halo, suggesting it may have a slight disturbance due to interactions with other nearby galaxies, however it does not look to be in any major merger. The color index suggests it is a redder, more evolved system.
