The galaxy presents as a largely smooth, featureless object, with a concentrated central bulge. Its overall shape is more elliptical than circular, tending towards a somewhat cigar-like form. There are subtle indications of a disk structure, but it does not dominate the galaxy's appearance. The color profile suggests a relatively evolved stellar population. There is no apparent evidence of ongoing major merger activity, but there is some slight indication of possible minor disturbances in the morphology.
