The galaxy presents as a centrally concentrated, yellow-hued object, suggesting a dominant older stellar population. It appears to exhibit a smooth morphology, with little evidence of spiral arms or significant dust lanes. The overall shape approximates a rounded structure, though a slight elongation is apparent. There's an indication of a minor disturbance or faint tidal feature extending from the main body, although the resolution limits a definitive assessment. The relative brightness of the galaxy implies a substantial stellar mass. A lack of significant blue light suggests a relatively low rate of ongoing star formation.
