The galaxy presents as a diffuse, lenticular or early-type spiral galaxy. It exhibits a smooth, concentrated light profile with minimal discernible structure. Its overall color suggests a low star formation rate, with a slightly redder hue indicative of an older stellar population. There is little evidence of prominent spiral arms or active star-forming regions. The galaxy appears relatively isolated, with no immediate signs of tidal interactions or mergers. It has a somewhat elliptical morphology, appearing more elongated than circular. Faint extensions might be present, but are not well-defined.
