The object presents as a relatively smooth, centrally concentrated galaxy, appearing largely elliptical in morphology. The light profile suggests minimal disk-like features. The color index indicates a relatively red population, consistent with an older stellar population and/or significant dust extinction. There is no apparent evidence of significant ongoing star formation, nor signs of strong tidal disturbance or recent merger activity in the immediate vicinity. The galaxy exhibits a high degree of roundness. Minor disturbances in the galaxy cannot be ruled out.
