The galaxy presents a generally elliptical morphology, though subtle features hint at the presence of a disk component. A concentrated, bright central bulge dominates the galaxy's luminosity profile. This bulge exhibits a yellowish-orange hue, suggesting a population of older stars. Moving outward from the core, a flattened disk structure becomes apparent. This region is bluer in color, which indicates the presence of younger, hotter stars and potentially ongoing star formation. There appears to be some dust and gas. The overall structure suggests a galaxy that is somewhere between a pure elliptical and a spiral type, possibly a lenticular galaxy (S0) or a spiral galaxy with tightly wound arms. There is a minor chance of an early stage merger or tidal disruption. The galaxy does not appear to be significantly disturbed or actively merging with another system based on the symmetry of the central bulge and outer disk.
