The galaxy presents as a relatively compact object with a somewhat elliptical morphology. The light profile appears smooth, lacking any readily discernible spiral arms or significant dust lanes. There is a subtle color gradient visible, transitioning from a predominantly redder hue in the central region to a slightly bluer periphery, indicating a possible difference in stellar populations. There is no evidence of any major tidal disturbances or ongoing merger activity, with no nearby companions clearly interacting with the system. Overall the galaxy appears to be a relatively evolved system, possibly a lenticular or early-type spiral galaxy seen at some distance.
