The galaxy presents a complex morphology, appearing as two distinct components. The primary component exhibits a smooth, elongated structure, suggestive of a spheroidal or elliptical galaxy. The color is predominately blue-white, possibly indicating a population of younger, hotter stars, with an estimated effective radius of about 4.6 kpc. The secondary component is more compact and yellow-orange, which would indicate a population of older stars, with an estimated mass of about 10^10 solar masses. A low star formation rate is indicated, though some star formation activity may be present. Evidence of past or ongoing minor gravitational interactions is present, potentially supported by the non-uniform structure. Overall, the galaxy seems to be transitioning towards a quiescent state, as seen by the intermediate colors and morphology.
