The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. There is little evidence of significant spiral arm structure or prominent dust lanes. The light profile appears relatively uniform, transitioning gradually from a bright central core to fainter outer regions. The overall color appears yellowish-white, suggestive of a stellar population dominated by older, redder stars, with possible low levels of ongoing star formation. There are no obvious signs of tidal disturbances, major mergers, or active galactic nucleus activity based on the image. The galaxy appears relatively undisturbed and well-defined within the limits of the image resolution. 
