The galaxy presents an elliptical morphology, displaying a relatively smooth light distribution without prominent spiral arms or distinct features. The central region exhibits a concentrated luminosity, suggesting the presence of a substantial galactic nucleus. Proceeding outward from the core, the light intensity gradually decreases, indicative of a diminishing stellar density. The overall color profile tends toward a slightly yellowish hue, implying a stellar population dominated by older, redder stars, characteristic of an evolved stellar system. Slight blue hints are visible in the outer halo. The axial ratio suggests a nearly circular shape, although a subtle elongation might be present. The morphology seems largely undisturbed, showing no signs of significant tidal interactions or ongoing mergers.
