The galaxy presents as a slightly elongated, lenticular-like system with a smooth, concentrated central bulge. The galaxy appears generally featureless, lacking any distinct spiral arm structures or prominent dust lanes. There is a color gradient, transitioning from a yellowish hue near the core to a bluer tint in the outer regions, suggesting a possible radial change in stellar populations and ages, with older stars concentrated towards the center and relatively younger stars in the periphery. The galaxy's overall morphology suggests a relatively quiescent system, although some minor disturbances or interactions cannot be ruled out based on the image alone. Overall the galaxy appears to be relatively massive. There is a modest amount of star formation occurring.
