The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population of older stars. There's little evidence of significant dust lanes or spiral arm structures; the light appears to be smoothly distributed throughout the galaxy's body. A slight elongation is perceptible, but it largely appears to be a rounded shape. There is no obvious presence of any active galactic nuclei or point source emissions. Possible minor disturbances or faint tidal features are very subtly suggested in the outer halo, though nothing significant. Overall, the galaxy seems to be in a relatively quiescent state, possibly a evolved system that has experienced a lull in star formation.
