The observed galaxy presents as a slightly elongated, elliptical morphology. The color profile exhibits a dominant yellow-orange hue concentrated toward the galactic center, indicative of an older stellar population. Minimal blue is present, suggesting a low current star formation rate. There are no prominent spiral arm structures or dust lanes discernible within the image. The overall smoothness of the light distribution further supports a classification leaning toward an elliptical galaxy type. There is a slight hint of asymmetry suggesting possible minor interactions or disturbances, though the primary structure appears generally undisturbed. The estimated size suggests it is likely a mid-sized galaxy.
