The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing bright yellowish-white, suggestive of an older stellar population. The galaxy's overall shape is somewhat elongated, but not markedly so, exhibiting a ratio of approximately 1:3. The outer regions exhibit a gradual decrease in brightness, fading into the background sky with no clear evidence of spiral arms or distinct features. There is a subtle color gradient from the center outwards, shifting towards redder hues in the periphery. No significant signs of recent mergers or major disturbances are immediately apparent in the image.
