The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its shape is close to circular, displaying little elongation or asymmetry. The light profile transitions gradually from a bright core to fainter outer regions. The color of the core appears yellowish-white, potentially indicating a population of older stars. A subtle bluish tint is observed in the outer regions which could signify areas of more recent star formation. There's no clear evidence of distinct spiral arms or a prominent disk structure. No major disturbances or ongoing merging events are apparent. The overall appearance suggests an evolved system, likely an elliptical or lenticular galaxy.
