This galaxy exhibits a predominantly elliptical morphology, elongated along its major axis. The central bulge appears luminous and yellowish, indicating a concentration of older stellar populations. Moving outward from the core, the light gradually diminishes, transitioning to a fainter, less defined halo. The galaxy appears relatively smooth in texture, with minimal evidence of significant spiral arm structures or prominent dust lanes. There is a slight indication of a disk-like structure, but it is much fainter and less prominent than the bulge. The galaxy does not appear to be undergoing any major merging events or showing signs of significant tidal disturbances, though a slight asymmetry in the outer regions could suggest minor gravitational interactions. The color gradients suggest a relatively quiescent star formation history. Overall, the galaxy appears to be a mature system, likely an elliptical galaxy with a dominant bulge.
