The galaxy presents a smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, displaying a gradual decrease in luminosity from the core outwards. The color profile suggests an evolved stellar population, appearing generally redder in comparison to galaxies with active star formation. There is no apparent evidence of significant ongoing star formation. No tidal features or obvious signs of recent mergers are visible. The galaxy exhibits a generally rounded shape, with no strong indication of being elongated or highly distorted. Any internal structures present are not clearly discernible at the given resolution.
