The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a concentrated, roughly spherical distribution, with a distinct central bulge and no prominent spiral arm structures. The core appears bright and yellowish-white, suggesting a population of older stars. Moving outwards from the center, the galaxy fades in brightness gradually. There is no distinct color change visible outside of the central bulge. The overall impression is of a relaxed system, not currently undergoing significant star formation activity. There is no morphological evidence of interaction with another galaxy or any disturbance.
