The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a high concentration of light, gradually decreasing towards the outer edges. The color profile suggests an older stellar population, with a noticeable redder hue dominating the galaxy's overall appearance. There is no evident spiral arm structure or significant dust lane obscuration visible in this image. The galaxy may have a very faint disk, but there is no prominent structure. There is some evidence of disturbance, with a small amount of apparent tidal debris, suggesting possible past or ongoing interactions with a companion galaxy.
