The galaxy exhibits a generally smooth morphology, with a central bulge that appears largely homogenous and featureless. This bulge transitions into a fainter disk, with a hint of a somewhat elongated or cigar-shaped overall form. The disk component shows some subtle irregularities, possibly indicative of minor disturbances, although no major merger events are evident. The galaxy presents a flattened spheroidal shape and its color suggests the presence of a mix of stellar populations, with a more pronounced concentration of older stars towards the bulge, and a hint of younger stars present in the bluer, less concentrated regions of the disk.
