This galaxy appears to be relatively compact, with an elliptical morphology. It exhibits a bright, concentrated central bulge region, which is roughly symmetrical. There is also a more diffuse region surrounding the central bulge, suggesting a possible galactic disk component. The color gradient shifts from blue to red further from the center of the galaxy. This possibly indicates the presence of a population of younger, hotter stars towards the center, and older, cooler stars residing in the outer regions. The distribution of light is largely smooth throughout the galaxy, with no apparent spiral arms or significant dust lanes visible. The overall shape appears undisturbed, with little evidence of tidal tails or other morphological irregularities that would indicate a recent merger event. There might be the slightest suggestion of a minor disturbance, perhaps a small amount of tidal debris visible in the outer regions.
