The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge, with the light intensity decreasing gradually outwards. The color profile suggests a population of older stars, with a yellowish hue dominating the galaxy's overall appearance. There is a slight elongation to the galaxy's shape, deviating from a perfectly circular form, presenting a somewhat cigar shaped look. No distinct spiral arms or dust lanes are discernible. There is no strong evidence of recent or ongoing major merger activity. The structure indicates a relatively evolved system.
