The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. Its light is dominated by warmer colors, shifting from yellow to orange towards the core, indicating an older stellar population and reduced levels of recent star formation. There is some indication of a subtle disc structure, though it lacks prominent spiral arms, suggesting an advanced stage of morphological transformation. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or major mergers. However, there may be minor disturbances present within the galaxy. Overall, the light distribution appears quite uniform, indicating a well-mixed stellar population. The overall size of the galaxy, relative to others in the field of view, suggests a significant physical extent.
