The galaxy exhibits a generally elliptical morphology, with an apparent flattening. Its color profile suggests an evolved stellar population, exhibiting a redder hue in the central regions, gradually fading into a bluer halo. There is a hint of faint, diffuse extensions, giving it a somewhat disturbed appearance. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively smooth in texture, without prominent dust lanes or knots of star formation. The light is centrally concentrated, indicative of a high concentration of stars towards the galactic core.
