The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a yellowish hue in its core. This suggests a significant population of older stars in the nuclear region. The overall shape appears somewhat rounded, though a slight elongation is discernible, hinting at a possible departure from a perfect elliptical morphology. There are subtle color gradients throughout the galaxy, with the inner regions displaying a more pronounced yellow color and the outer regions tending toward a redder or more diffuse appearance. There are no distinct spiral arms or obvious signs of active star formation readily apparent. The galaxy appears to be undergoing some sort of merging event, or has recently been through a significant interaction, causing a disturbance in the morphology.
