The galaxy exhibits a morphology that appears intermediate between elliptical and spiral. There is evidence of a disk structure, though it's not as clearly defined as in typical spiral galaxies. The overall form is somewhat elongated, neither perfectly spherical nor highly flattened. A smooth component is noticeable, suggesting a significant population of older stars. The galaxy shows signs of a potential interaction or merger event; there is some visible distortion in its shape with possible tidal features present. Star formation activity appears to be relatively low, and the galaxy is quite massive. The colour suggests the existence of a number of older stars, implying that most of the recent star formation has been quiescent.