The galaxy presents a generally smooth, elliptical morphology. The color profile suggests a relatively old stellar population, with a dominant yellowish-orange hue concentrated towards the center. There is minimal evidence of spiral arm structure or significant dust lanes. The light is centrally concentrated, with a gradual decrease in brightness as the radius increases. No strong tidal features or signs of recent major merger activity are apparent; it seems relatively undisturbed. There may be minimal ongoing star formation, given the slight bluer tinge at the edges of the galaxy, but it appears to be occurring at a low rate. The overall form is nearly circular, tending slightly toward a cigar shape.
