The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, tending towards a rounded form rather than a highly elongated or cigar-shaped structure. There is some suggestion of a disk-like component, but it is faint and not well-defined. A slight color gradient is visible, transitioning from a bluer hue in the outer regions to a yellower or whiter core. This color profile suggests a stellar population that is younger in the outer regions, potentially indicating ongoing star formation. There are no obvious signs of major mergers or significant tidal disturbances affecting the structure of the galaxy. Overall, the galaxy presents as a relatively undisturbed, evolved system with a dominant spheroidal component.
