The galaxy presents as an elliptical morphology, with a smooth, largely featureless appearance. The central region exhibits a higher luminosity, indicated by its brighter, yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward, the galaxy fades gradually, maintaining its elliptical shape. There's a subtle transition in color toward the outer edges, showing a slight shift to a redder tint, potentially hinting at a difference in the age or composition of the stars in these regions. No distinct spiral arms, dust lanes, or irregular structures are discernible. The overall shape suggests a relatively relaxed and evolved system.
