The object presents as a moderate sized galaxy, roughly elliptical in appearance, though some irregularities are noted. The core region exhibits high surface brightness, with a strong concentration of light indicating a relatively dense stellar population. The galaxy shows a redder hue, indicative of older stellar populations, although there are hints of a slight bluer region possibly of newer star formation. The overall smooth appearance suggests that the galaxy may be an elliptical galaxy, but cannot rule out a spiral viewed edge-on. There may be minor disturbances from a recent merger, though this is not definitive. 
