The galaxy presents as a single, relatively smooth object with a central concentration of light. It exhibits an elliptical morphology, appearing as a flattened spheroid, with the semi-major axis oriented roughly horizontally in the image. The galaxy's light is dominated by a bright, unresolved core which fades gradually into the outer regions. Color gradients are subtle but detectable, transitioning from a blueish-white core to slightly redder hues in the outer halo. There is no visible spiral arm structure or significant dust lane obscuration. The generally smooth appearance suggests a relatively evolved system where ongoing star formation is low. The roundness of the galaxy's profile indicates that it is likely closer to an elliptical galaxy rather than a highly inclined spiral galaxy. The lack of any obvious tidal features or distortions suggests that it is not currently undergoing a major merger event, but could have experienced minor disturbances in the past.
