The galaxy appears as a moderately luminous object exhibiting a generally smooth morphology. There appears to be some presence of a disk, but the overall structure suggests a somewhat spheroidal shape, transitioning between round and elliptical. The galaxy exhibits a color gradient, with a yellowish-orange hue at the center, transitioning to redder tones, which indicates older stellar populations. There is no obvious spiral structure visible, and the galaxy lacks prominent features such as dust lanes or active star-forming regions. There is a possibility the galaxy is undergoing or has recently undergone a minor merger event, as it appears to be slightly disturbed. 
