The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There is a slight elongation in the morphology, but it does not appear highly flattened. The color profile suggests a relatively evolved stellar population, with a subtle reddening towards the core of the galaxy. Faint, diffuse extensions are possibly present, but not clearly defined from the main body of the galaxy. There does not appear to be significant evidence of a spiral structure, prominent dust lanes, or ongoing major merger activity. Any star forming regions appear to be absent or significantly diminished.
