The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. There is an apparent lack of significant spiral arm structure or prominent dust lanes. The central region is more luminous, indicating a higher concentration of stars toward the galactic core. There is a color gradient visible, transitioning from a yellowish hue in the center to a redder tinge in the outer regions, which may indicate an aging stellar population as you move from the galactic center outwards. No signs of strong tidal disturbance or merging activity are immediately apparent. Overall, the galaxy's smooth morphology and color profile suggest it is a relatively evolved system.
