The galaxy presents as a relatively smooth, elliptical structure with a prominent bulge. The core exhibits a concentrated, bright yellowish-white hue, indicating a high density of older stellar populations. Moving outward from the core, the light gradually fades into a more diffuse, reddish-orange halo. The galaxy's overall shape is slightly elongated, appearing closer to an oblate spheroid than a perfect sphere, suggesting some degree of rotation. There is no distinct dust lane or spiral arm structure visible. Subtle irregularities in the outer halo may indicate minor gravitational interactions or past mergers, although the primary structure appears undisturbed. Overall, the galaxy appears to be a massive, evolved system with a well-established morphology.
