The galaxy presents as a lenticular or possibly elliptical structure. Its morphology appears generally smooth, lacking prominent spiral arms or distinct features suggestive of active star formation. The galaxy exhibits a noticeable elongation, approaching a cigar shape. The color profile is fairly uniform, displaying a yellowish hue, which typically indicates an older stellar population. The galaxy shows no signs of major disturbances or ongoing merging events. There is evidence of a potential smaller satellite galaxy nearby. This galaxy may be interacting with the primary structure.
