The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a radial falloff in luminosity, suggestive of an older stellar population. The color profile indicates a dominant red-yellow hue in the core region, transitioning to a bluer periphery. There appears to be little evidence of distinct spiral arms or significant dust lanes. The overall morphology suggests a high degree of central concentration. Based on its color and morphology, star formation rates are likely moderate, with an estimated intermediate stellar mass. There are no apparent signs of major mergers or tidal disturbances. The shape tends toward round, with a slight departure.
