The galaxy presents as a relatively compact, elliptical morphology. It displays a smooth, mostly featureless profile, lacking prominent spiral arms or a well-defined disk structure. Its overall shape is quite round, with a low degree of elongation or asymmetry. There is no obvious central bulge; instead, the luminosity seems evenly distributed. The light is dominated by reddish-yellow hues, suggestive of an older stellar population. No significant dust lanes or active star-forming regions are apparent within the galaxy's body, implying a low star formation rate. Some minor disturbances may exist in the galaxy's profile, however it mostly appears non-merging. 
