This galaxy exhibits a predominantly smooth morphology, appearing as a relatively featureless elliptical. It presents a bright, concentrated core that gradually diminishes in intensity outwards. The overall shape is elongated, exhibiting a cigar-like morphology. Faint indications of a possible disk component can be seen around the center of the galaxy. There is no major evidence of any recent or ongoing major merging events, although some minor disturbances could be present. The light emitted suggests the presence of some ongoing star formation, with an average mass and a stellar population of intermediate age. The size indicates that it is relatively large.
