The galaxy presents as an elliptical morphology, with a smooth, diffuse appearance. The light is concentrated towards the center, indicating a strong bulge component. The color gradient suggests that the central region is populated by older stars. The galaxy does not display any prominent spiral arms or distinct features. It appears relatively undisturbed. The light distribution is elongated, with an ellipticity of approximately 0.6. The image lacks any clear indications of significant ongoing star formation.
