The galaxy presents as a system with two distinct, interacting components. One component exhibits a smooth, elliptical morphology, with a concentrated, yellowish hue suggesting an older stellar population and relatively low star formation activity. The second component appears smaller, bluer, and less defined, potentially indicating a region of active star formation or a smaller, infalling dwarf galaxy undergoing tidal disruption. There appears to be a disturbance in the overall structure, hinting at a possible ongoing or recent merger event between the two components. The roundness indicates the galaxy is not highly elongated. Evidence suggests the components are exhibiting gravitational interaction with each other.
