The galaxy presents a largely smooth morphology, with an elliptical or lenticular-like appearance. The light distribution is centrally concentrated, exhibiting a moderate degree of roundness. There's little evidence of spiral arms or a prominent disk structure, though subtle color gradients suggest potential underlying complexity. No signs of ongoing major mergers or significant tidal disturbances are apparent in the immediate vicinity, though very minor asymmetry cannot be excluded. The overall color profile suggests a relatively old stellar population, likely with moderate ongoing star formation. The galaxy exhibits a moderate redshift.
