The galaxy presents as a luminous, centrally concentrated object with an apparent elliptical morphology. The light distribution appears relatively smooth, lacking prominent spiral arms or significant dust lanes. The color profile suggests a population of older stars, with a redder hue observed towards the galactic core and a slight shift towards blue on the outer edges. The object appears elongated, approximately three times longer than it is wide. There is no obvious evidence of tidal disturbances or ongoing major merger events. The galaxy presents a classical elliptical morphology.