The galaxy presents as a relatively smooth, elliptical or lenticular type, exhibiting a concentrated central bulge that gradually diffuses outward. There is little evidence of spiral arm structure or distinct features, suggesting a lack of significant ongoing star formation. The overall color appears to be yellowish or reddish, indicative of an older stellar population. It appears quite round in shape and shows no signs of interaction or merging events. A very faint halo may be present, extending slightly beyond the primary body of the galaxy. 
