The galaxy presents as a generally smooth, elliptical or lenticular system. It appears to be moderately inclined with respect to our line of sight. The color distribution suggests an older stellar population, with a relatively redder appearance overall and a smooth light profile, indicating a lack of significant ongoing star formation. There is some evidence of minor disturbances but these do not suggest a major merging event is occurring. The galaxy's morphology is consistent with it being a mature system, potentially with a high stellar mass. The overall structure hints that the galaxy is relatively undisturbed and has likely been evolving passively for a significant amount of time.
