The galaxy appears to be a relatively smooth, single object, with a generally elliptical morphology. The primary body exhibits a concentrated, yellowish-white core, suggesting a substantial population of older stars. There are some subtle features, especially a hint of reddish emission to the south of the core which may be a region of more active star formation, although the majority of the galaxy is characterized by relatively quiescent star formation. The overall structure indicates that it is likely an early-type galaxy without well-defined spiral arms. There does not appear to be any evidence of major mergers, though subtle minor disturbances cannot be excluded. The object seems to be more round than cigar shaped. 
