The galaxy presents as a relatively smooth object with a subtle disk-like structure, exhibiting a slight elongation. The color profile suggests an evolved stellar population, potentially indicating a lower rate of star formation. There is a hint of a possible minor disturbance or tidal feature in the form of a very faint asymmetry. The overall morphology appears to be somewhere between round and in-between, leaning more towards round. It does not appear to be actively merging.
