The galaxy appears as a somewhat elliptical, smooth object. The core region exhibits a bright, yellowish-orange hue that gradually fades into a bluer, less distinct outer region. There is little evidence of spiral arms or significant dust lanes. The overall structure suggests a relatively evolved system, potentially an early-type galaxy. There is a very slight hint of tidal disturbance around the galaxy, likely due to a minor merger in its recent past. The galaxy has a relatively concentrated luminosity profile, with the highest intensity light emitted from the central region.
