The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution appears uniform, lacking prominent spiral arms or distinct features indicative of ongoing major star formation. There's a subtle color gradient from the center to the outer regions, with the core appearing slightly bluer. There are some indications of minor disturbances, though the object does not obviously appear to be undergoing a major merger. Based on its color and smooth structure, this galaxy likely has a relatively low star formation rate.
