The galaxy presents as a largely featureless, elliptical morphology. There is a concentrated central bulge with a smooth luminosity profile that diminishes with radial distance. The galaxy is slightly elongated and exhibits a fairly high degree of rotational symmetry. There is a lack of discernible spiral arm structure or significant dust lanes within the visible wavelengths. The color is somewhat homogenous throughout the galaxy with a slightly yellow/white hue, indicating the presence of an older stellar population. There is no evidence of recent or ongoing major merger events.
