The galaxy presents as a centrally concentrated, relatively smooth object, with an approximately elliptical morphology. A bright core dominates the galaxy's central region, surrounded by a diffuse, extended halo. The color profile appears to exhibit a slight gradient, transitioning from a more yellow/red hue in the core to a somewhat bluer tint in the outer regions of the halo. There is no clear evidence of spiral arm structures or significant dust lanes. The overall appearance suggests a galaxy towards the redder end with relatively high mass and low star formation rate. There is no apparent evidence of interaction or major morphological disturbance.
