This galaxy appears to be a relatively luminous, early-type galaxy, potentially an elliptical or lenticular type. The core exhibits a concentrated brightness profile, characterized by a yellowish-orange hue suggesting an older stellar population. A subtle extension of light surrounds the central region with a slight flattening, possibly indicating a disk component or tidal features. The outskirts of the galaxy display a bluer tint, hinting at the presence of younger stars or ongoing star formation, albeit at a low rate. There are no prominent spiral arms or dust lanes visible, indicating a smoother, less structured morphology. Overall, the galaxy appears relatively undisturbed, with no signs of a major merger event.
