The galaxy presents as a moderately compact object, exhibiting a centrally concentrated light profile. Its morphology is generally smooth with a nearly round shape, showing little indication of spiral arms or a pronounced disk structure. The core region appears bright and somewhat yellow/gold in color, likely indicative of an older stellar population. A subtle blue halo surrounds the central region, hinting at the presence of younger stars or ongoing star formation, albeit at a modest rate. There is no visual evidence of significant tidal disturbances or ongoing major mergers. Slight asymmetry may be present, but further analysis would be required to determine the nature of this.
