The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears elliptical, with no obvious spiral arms or bar structures visible in this imaging. The light distribution exhibits a radial gradient, with the brightest intensity concentrated at the center and gradually fading outwards. There are no distinct features indicative of a recent major merger event, though subtle asymmetries in the outer regions cannot be entirely ruled out. The galaxy's color profile suggests a population of older stars, as indicated by the reddish-yellow hue, particularly towards the central regions. No significant dust lanes or prominent star-forming regions are apparent. The lack of distinct features and relatively smooth light distribution suggest that this galaxy is a relatively quiescent system.
