The galaxy presents a primarily smooth morphology, exhibiting a centrally concentrated luminosity profile. There is a subtle indication of a potential disk-like structure but this is difficult to confirm due to the galaxy's overall smoothness. The colour profile appears slightly redder in the central region, potentially indicating an older stellar population or the presence of dust obscuration. There is evidence of a small amount of ongoing star formation, which appears concentrated towards the outer regions of the galaxy. There may be some minor disturbance or interaction occurring, although the features are not prominent, indicating that if a merger is occurring, it may be in its late stage. The overall shape is close to round.
