The galaxy presents a generally smooth, rounded morphology, with a slight deviation from perfect circularity. A dominant central bulge is visible, exhibiting a concentrated luminosity. The galaxy appears to lack well-defined spiral arms or prominent disk features. There is some indication of minor disturbances, but the overall structure remains relatively undisturbed. The color profile suggests a population of older stars and a relatively low rate of ongoing star formation, as indicated by the redder hues. This galaxy is reasonably massive, possibly suggesting that it is an elliptical galaxy. 
