The galaxy appears to be an elliptical galaxy due to its smooth light distribution. It is circular, with a slight orange hue, potentially indicating an older stellar population. No distinct features, spiral arms, or dust lanes are visible, suggesting a lack of ongoing major star formation. The galaxy exhibits a concentrated central bulge with a gradual decrease in light intensity towards its outer regions. There are no signs of tidal tails or disturbances, meaning it does not seem to be undergoing any significant interactions with other galaxies.