The galaxy presents a largely smooth and relatively featureless morphology. It appears elliptical in shape, with a high degree of central concentration. The color profile suggests an older stellar population, trending toward redder wavelengths. There is little evidence of significant spiral arm structure or prominent dust lanes. Faint extensions may be present, indicating possible tidal interactions or recent minor disturbances, although the overall structure seems undisturbed. The light distribution is centrally concentrated, with intensity gradually decreasing towards the edges, giving it a diffuse appearance.
