The galaxy presents a generally elliptical morphology, with a smooth light distribution lacking prominent spiral arms or a distinct central bar. The light profile appears centrally concentrated, with a gradual decline in surface brightness moving outward from the core. The core exhibits a reddish hue, possibly indicative of an older stellar population or significant dust obscuration. Surrounding the core is a more diffuse, greenish-white halo, suggesting a population of younger stars and ongoing star formation. No obvious tidal features or other signs of recent major mergers are apparent, though subtle irregularities in the outer isophotes cannot be ruled out at this resolution. Based on the observed characteristics, this galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy.
