The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is concentrated towards the center, suggesting a prominent bulge component. The galaxy exhibits a yellow-red hue, which implies an older stellar population and a relatively low rate of on-going star formation. There appears to be a secondary, smaller mass object nearby. It is difficult to tell without higher resolution if this is a second nucleus from a recent merger or a different galaxy close by. While the galaxy appears mostly undisturbed, there appears to be some tidal interaction.
