The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. It exhibits a notable absence of distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, indicated by a yellow-orange hue. There are no visible signs of ongoing major mergers or tidal disturbances in the immediate vicinity. The overall morphology suggests a classification towards the early-type galaxy sequence. The galaxy exhibits a round shape. There is no evidence of distinct star formation activity within the observable light.
