The galaxy appears to be an elliptical type, exhibiting a largely smooth and featureless morphology. It presents with a centrally concentrated luminosity profile, suggesting a prominent bulge. The overall shape is mostly rounded and without any sharp edges. A subtle color gradient is noticeable, shifting from a yellow-orange hue in the central region to a slightly bluer tint in the outer regions. No clear spiral arms or dust lanes are visible within the galaxy, indicating a lack of significant ongoing star formation in the central regions. There does not seem to be any evidence of tidal tails, bridges, or disrupted morphology suggesting recent major merger events. However, there appears to be some minor asymmetry, suggesting minor disturbances.
