The galaxy presents as a relatively smooth, elongated object, exhibiting a cigar-like shape. Its central region appears to be a spheroid of moderate concentration, and exhibits a bright central peak. Faint, diffuse emission is observed along the galaxy's major axis, suggesting the presence of a disk component. There is no strong evidence of significant recent or ongoing mergers or tidal disturbances, however a small blue spot is present at the very center of the galaxy, this may indicate either a supermassive black hole, or small amounts of star formation. The galaxy's overall color index indicates a population of older stars, though with some evidence of recent, but low levels of star formation.
