The galaxy presents as a well-defined elliptical or lenticular structure. Its light profile appears relatively smooth, lacking any prominent spiral arms or irregular features. The galaxy's overall shape appears to be elongated, suggesting a deviation from perfect sphericity, perhaps closer to an "in between" roundness. There is no clear visual indication of a major ongoing merger, though subtle tidal features cannot be ruled out completely at this image resolution. The galaxy exhibits a moderate blue color, hinting at ongoing star formation, albeit at a relatively low rate. This low rate of star formation would imply that the galaxy consists primarily of older stellar populations.
