The galaxy presents a relatively smooth, elliptical morphology. It displays a concentrated central bulge that dominates its overall structure. The color profile suggests a population of older stars, although there appears to be a small degree of on-going star formation, particularly in the inner regions, indicated by the presence of slightly bluer light near the core. The galaxy appears generally undisturbed, with no obvious signs of tidal interactions or major mergers. It exhibits a moderate degree of roundness in its shape, leaning more towards an intermediate elliptical classification rather than a highly spherical one. There is a hint of a faint, extended halo surrounding the main body of the galaxy, though its boundaries are poorly defined. The galaxy is not perfectly uniform; closer inspection reveals some subtle variations in light distribution throughout its body.
