The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is little evidence of spiral arm structure. The galaxy appears to be somewhat lenticular, neither perfectly elliptical nor displaying strong disk features.

The colouration suggests ongoing star formation, with bluer regions visible, although these are not sharply defined. The overall colour index indicates a relatively mature stellar population. The galaxy exhibits some signs of minor disturbances, possibly indicative of a past or ongoing interaction. There do not appear to be any major mergers occurring at this time.
