The galaxy presents as a relatively smooth, yet not entirely featureless, structure. It has a central, bright bulge which is slightly elongated. There is a suggestion of a faint, diffuse disk surrounding this central region. The overall shape is not perfectly round, leaning toward an intermediate elliptical morphology. There may be slight disturbances in its morphology, hinting at a possible minor interaction or past merger event, though the galaxy appears largely undisturbed. The galaxy exhibits a color gradient, appearing bluer in the outer regions of the disk and redder towards the central bulge. This suggests a difference in stellar populations, with younger, hotter stars populating the disk, and older, cooler stars residing in the bulge. Overall, the galaxy appears to be a relatively quiescent system, not undergoing significant active star formation at the present time.
