The galaxy exhibits a generally smooth morphology, with a highly concentrated central region that emits strongly in the observed red and green bands, indicating a potentially older stellar population. The overall shape appears somewhere between round and elliptical. There is very little evidence of spiral arm structure or significant dust lanes. There are no signs of ongoing or recent major merger activity, though minor tidal disturbances cannot be ruled out from this image alone. Given its redder color, and lack of disk structure, this galaxy may exhibit relatively little current star formation activity.
