The galaxy exhibits a generally elliptical morphology, with a smooth and concentrated central bulge. The light profile appears to follow a Sersic distribution, with the light concentration somewhat centrally focused. The galaxy is not perfectly circular, it appears slightly elongated. There is a marginal dust lane/disk like structure near the center of the galaxy, that runs from the bottom left of the galaxy to the top right, though it is not fully visible with the current image and more observations are needed. The galaxy's color indices indicate a bluer central region compared to its periphery, suggesting a modest level of on-going star formation activity within the central core. The outer regions are considerably redder. There is no visually apparent evidence of any major merging events or tidal disturbances affecting the overall structure, though minor disturbances cannot be ruled out. The overall impression is that of a well-established galaxy, undergoing moderate levels of stellar evolution.
