The galaxy appears as a roughly elliptical, well-defined object with a smooth light distribution. Its central region exhibits a concentrated, bright core that appears to be yellowish or golden. This color suggests an older stellar population. The outer regions of the galaxy display a gradual decrease in surface brightness and a subtle shift toward bluer colors, hinting at the presence of a younger stellar population, or a low level of on-going star formation. No prominent spiral arms or bar structures are discernible. There is a slight asymmetry in the outer halo, suggesting possible minor tidal interactions or recent accretion events. Overall, the galaxy presents a morphology consistent with that of an early-type galaxy, likely an elliptical, at an estimated distance corresponding to a redshift of roughly 0.25. The galaxy appears to be relatively undisturbed with no major merger events underway.
