The galaxy presents a generally smooth appearance, indicative of an elliptical or lenticular morphology. There is no apparent spiral structure. The galaxy is relatively round, with a slight deviation from perfect circularity. There is no obvious evidence of a major merger or significant tidal disturbance. The galaxy exhibits a centrally concentrated brightness profile, fading smoothly towards the edges. Color gradients within the galaxy suggest some level of stellar population variation. The galaxy appears moderately red. This color suggests a population of older stars with lower rates of current star formation. Overall, the galaxy appears to be a fairly evolved system with characteristics consistent with a high mass, and little to no current star forming activity.
