The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density or possible active galactic nucleus. The light distribution gradually diminishes from the core outwards, with no distinct spiral arm features visible. There is a slight elongation to the galaxy's shape, leaning towards an oblate spheroid appearance rather than a perfectly circular one. The color profile appears generally homogenous, with a subtle bluer tint in the outer regions compared to the yellowish-white core. There is no apparent evidence of major mergers or significant tidal disturbances in the immediate vicinity, although there may be minor asymmetry in the outer halo of the galaxy. The galaxy presents itself as a single, cohesive object with no obvious signs of recent major interactions.
