The galaxy presents as a centrally concentrated object with a smooth overall appearance. The morphology suggests a likely elliptical classification, exhibiting a generally rounded shape with a slight elongation. The central region displays a bright, concentrated core. The color profile indicates a significant presence of older stellar populations, contributing to the reddish-yellow hue. There are no distinct spiral arm structures or significant dust lanes visible. Faint, diffuse extensions of light are observed around the central core, indicating a gradual decrease in stellar density with increasing distance from the center. No obvious signs of major merger activity are apparent. The galaxy may be experiencing minor gravitational interactions, as suggested by a subtle asymmetry in its outer regions.
