The galaxy presents as a centrally concentrated, relatively smooth structure, appearing elliptical in shape. The core exhibits a bright, diffuse glow, transitioning outward into a fainter halo. The overall color gradient suggests a population of older stars, with a dominant yellowish-orange hue. There is very little evidence of spiral arm structure or significant dust lanes. It seems to be relatively isolated. Its light appears redshifted by a modest amount indicating its intermediate distance from us. The galaxy exhibits very little evidence of active star formation. There are no obvious signs of recent major merger events or significant tidal distortions, although some minor asymmetries cannot be ruled out due to the image resolution.
