This galaxy presents as a relatively smooth, elliptical-like object with a bright, concentrated central bulge. The light distribution appears centrally condensed, transitioning smoothly outwards from the core. There is a slight elongation, suggesting it is not perfectly spherical. The galaxy exhibits a subtle color gradient; the central region appears slightly redder than the outer regions. This hints at a more evolved stellar population dominating the core, while younger, bluer stars may be more prevalent in the outskirts. There is no distinct evidence of spiral arm structure or significant dust lanes within the galaxy's morphology. Overall, the galaxy gives the visual impression of being a settled, relatively quiescent system.
