The galaxy presents as a luminous, centrally concentrated object. Its morphology appears predominantly smooth and elliptical, with a high degree of roundness. There is a gradual decrease in surface brightness from the core outwards, with no distinct spiral arm structures or prominent dust lanes discernible in the image. The color profile suggests a likely evolved stellar population, with a subtle reddening observed towards the central region, possibly indicative of older stars. The overall appearance suggests a system without significant ongoing major merger activity, possibly only exhibiting minor interactions. The estimated size of the galaxy places it within the range of intermediate-sized galaxies. The galaxy shows a detectable level of star formation activity.
