The galaxy appears as a moderately bright, relatively compact object. The morphology is largely smooth and elliptical, with a high degree of central concentration. A faint, diffuse halo surrounds a brighter, more spherical core. There is little indication of spiral arm structure or prominent dust lanes. The galaxy exhibits a redder color profile, suggesting an older stellar population with suppressed star formation. This indicates it has gone through the process of quenching or is red and dead, and is now less actively forming new stars. Overall, this galaxy presents as a fairly regular, evolved system.
