The galaxy presents as a somewhat elongated spheroid, exhibiting a smooth and relatively featureless appearance. The color profile suggests a predominantly older stellar population, with a bias towards redder wavelengths. There is a slight hint of bluer components in the central region, potentially indicating some ongoing star formation. The galaxy shows no strong evidence of spiral arm structure or significant dust lanes. There is a minor asymmetry to its shape. The overall morphology indicates a system that is likely in a late stage of evolution, trending towards an elliptical classification.
