The galaxy presents as a somewhat diffuse elliptical morphology. It exhibits a concentrated central bulge, fading into a more extended halo. The color profile suggests a population of older stars, appearing primarily yellow/red. There is no apparent dust lane or significant ongoing star formation regions visible in this image. No signs of recent merger activity are observable, such as tidal tails or distortions in the overall shape. The structure appears relatively smooth and undisturbed.
