The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. A bright central bulge dominates the galaxy's overall appearance, gradually fading outwards into a less distinct halo. The galaxy is generally round in shape. There is a subtle color gradient, transitioning from a yellowish-white hue at the core to a slightly redder tone in the outer regions. No prominent dust lanes or spiral arm structures are apparent. The overall structure suggests a relatively evolved system, potentially nearing the end of its star formation phase, consistent with an older stellar population dominating the observed light. There are no signs of major interactions or mergers.
