The galaxy presents a generally smooth, rounded morphology, with a concentrated central region of high luminosity. The core exhibits a yellowish-white hue, suggesting a population of older stars. Extending outwards from the core is a more diffuse halo, with a subtle transition in color towards blue. This may indicate a younger stellar population compared to the core, possibly influenced by ongoing star formation. Faint traces of what could be spiral arm structures appear in the outskirts of the galaxy, but they are poorly defined, implying a classification that trends toward elliptical or lenticular. There is a slight asymmetry in the light distribution, potentially signaling a past minor interaction or disturbance.
