The galaxy presents as a centrally concentrated, elliptical morphology. It is predominantly smooth in texture, with a notable lack of distinct spiral arms or prominent dust lanes. The color gradient suggests a population of older stars, exhibiting a yellow to reddish hue, which intensifies towards the core. The galaxy's overall shape is moderately round. There appears to be no evidence of ongoing major merger activity or significant tidal disturbances. It exhibits characteristics consistent with an early-type galaxy that may be undergoing a relatively low rate of star formation.
