The galaxy appears to be an elliptical or lenticular type, exhibiting a largely smooth morphology with a central bulge. The galaxy presents a slightly elongated shape. The color profile suggests a population of older stars, indicated by the yellowish to reddish hue, likely corresponding to a low rate of on-going star formation. There is no apparent dust lane or spiral arm structure visible. The outskirts of the galaxy appear diffuse, gradually fading into the background sky. There does not appear to be any signs of a major merger in progress.
