The galaxy presents as a somewhat centrally concentrated, elliptical morphology with a relatively smooth appearance. There is a slight elongation, but it is largely spheroid. The color profile suggests an older stellar population. The core region exhibits a bright, yellowish-white hue that diminishes gradually outwards, implying a concentration of older stars within its central region. There are no discernable spiral arm structures. The faintness of the outer region indicates low star formation activity. There are no indications of any major disturbances, suggesting a settled morphology, but there is evidence of possible minor disturbances and ongoing interaction. The galaxy does not have distinct features such as dust lanes or knots of star formation. Overall, the galaxy appears as a well-formed system in a state of late-stage evolution.
