This galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. It exhibits a generally rounded morphology, with a slight deviation toward a more elongated shape. The color profile suggests a population of older stars, primarily emitting in the redder wavelengths, as indicated by its orange/yellow hue. There is no significant evidence of spiral arms or other disk-like structures. No obvious signs of recent or ongoing major merger activity are visible, and the structure seems mostly undisturbed, with an appearance consistent with a relaxed system. The overall light distribution is centrally concentrated, indicating a large bulge component, and the galaxy appears to be relatively isolated based on the surrounding area.
