The galaxy appears as a relatively smooth, elliptical object with a concentrated central bulge. The color profile suggests an older stellar population, with a yellow-red hue dominating the central region. There is a marginal detection of bluer light on the outer edges, suggesting a very small amount of younger stars exist. The galaxy's light distribution is highly centrally concentrated and lacks any distinct spiral arm structures. A small portion of the galaxy is cigar shaped, but is mostly found to be in between round and cigar shaped. There are no signs of any major mergers or major disturbances of note. The overall morphology is that of a galaxy with depleted gas reserves and limited star formation.
