The galaxy exhibits a somewhat elongated, cigar-like shape, with a dominant, centrally concentrated bulge. There is evidence of a disk component, though it appears relatively faint and somewhat disturbed. The overall color of the galaxy leans towards red, indicating a population of older stars. Despite the redness, there is some presence of bluer light particularly in the central region, potentially suggesting some ongoing star formation or a younger stellar population in that region. There is also some slight evidence of interactions, or a possible close companion. There appears to be some asymmetry in the outer regions which may be evidence of disturbance.
