The galaxy appears to be an elliptical morphology, displaying a smooth, concentrated luminosity profile. The core region exhibits the highest surface brightness, gradually decreasing towards the outer regions. There is no prominent disk structure or spiral arm features visible. The galaxy exhibits a subtle ellipticity; its shape is slightly elongated. The color profile suggests an older stellar population, based on the redder hues. No significant signs of ongoing star formation or dust lanes are immediately apparent in this image.
