The galaxy presents a largely elliptical morphology, with a smooth light distribution. There is a slight elongation. The core of the galaxy exhibits a higher concentration of light, displaying a luminous yellow-orange hue, suggesting an older stellar population and/or significant dust obscuration. The outer regions of the galaxy show a more diffuse profile, and are subtly redder in color, which could indicate a lower density of star formation activity or a population of cooler stars. There is no clear evidence of spiral arms or a prominent disk structure. There may be a minor tidal feature present. The morphology suggests the galaxy is unlikely to be currently undergoing a major merger, but could be experiencing a minor disturbance.
