The galaxy presents a largely smooth morphology with a central, brighter region. This suggests it is likely an early-type galaxy, potentially an elliptical or lenticular, given the lack of prominent spiral arms. The galaxy displays a moderately flattened shape, somewhere between round and elongated. A subtle hint of a disk-like structure may be present, as indicated by a slight extension in one direction. There is no visible evidence of ongoing major mergers or significant tidal disturbances, but a possible minor asymmetry exists, suggesting past interaction or minor merging event. The overall color of the galaxy appears relatively red, which would indicate an older stellar population with a low star formation rate. This is supported by the smooth texture and lack of prominent blue regions typically associated with young, massive stars.
