The galaxy presents as an elliptical or lenticular structure, exhibiting a smooth, generally featureless morphology. The central bulge is pronounced, displaying a concentrated, yellowish-orange hue, suggestive of an older stellar population. An asymmetric extension is observed, possibly indicative of a tidal tail or debris field. The color gradient within this feature shifts towards the redder end of the spectrum, potentially signifying dust extinction or an older stellar population. No clear spiral arm structures or prominent dust lanes are discernible. The overall appearance suggests a system that has undergone, or is undergoing, a minor interaction or merger event.
