The galaxy presents a primarily smooth, elliptical morphology, though subtle features suggest the presence of a disk component. A concentrated central bulge, exhibiting a yellowish-orange hue, dominates the galaxy's structure. Fainter, bluish light extends outward from the core, indicating the presence of a younger stellar population within what appears to be a flattened, disk-like structure. The galaxy exhibits a moderate degree of roundness, leaning towards an in-between classification rather than perfectly spherical or elongated. There is no clear indication of ongoing major merging activity, though minor disturbances or asymmetries cannot be entirely ruled out at this resolution. Overall, the galaxy appears to be a mature system undergoing relatively low levels of star formation.
