The galaxy appears to be a relatively compact, elliptical type. Its overall form is smooth and rounded, with a high degree of central concentration, though a slight extension seems to be appearing to the lower side of the galaxy. The galaxy presents a dominant yellowish-white hue, suggestive of an older stellar population. Faint reddish coloration is observed to the lower side of the galaxy, indicative of possible on-going star formation, dust, or a population of older, redder stars. There are no apparent spiral arm structures or significant dust lanes visible. The overall morphology suggests the galaxy may be approaching a passive evolutionary state. There appears to be a small amount of disturbance nearby, perhaps suggesting a minor interaction.
