The galaxy appears to be relatively compact with an apparent size of approximately 6 arcseconds across. Its morphology is somewhat amorphous with a high degree of central concentration. A bright, cyan-colored core region is visible, surrounded by a less intense, more diffuse envelope. There is evidence of some asymmetry within the galaxy's outer regions, indicating that it is more complex than a standard elliptical galaxy. Patches of redder emission are visible, distributed in a ring like fashion around the brighter central region. These may be indicative of dust lanes or regions of active star formation. Overall, the galaxy's light profile suggests a blend of both smooth and more disrupted features. The galaxy shows signs of a possible minor disturbance or interaction, which would explain the asymmetry in the outer halo. It is plausible that this is either a recent interaction, or the late stages of a merger.
