The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, diffuse light distribution, lacking prominent spiral arms or a well-defined disk structure. The core region is characterized by a bright, concentrated luminosity, suggesting a significant stellar density. Moving outward from the core, the luminosity gradually decreases, forming a faint, extended halo. There is evidence of a slight bluing in the outer regions which may be due to the presence of younger stars or ongoing star formation. No significant tidal features or signs of recent major mergers are discernible in the image. The object appears largely undisturbed.
