This galaxy exhibits an overall elliptical morphology, appearing relatively smooth in texture. The central region displays a bright, concentrated core, indicative of a possible galactic nucleus. Moving outward from the core, the luminosity gradually decreases, suggesting a diminishing stellar density. The color gradient shifts subtly from a warmer, yellowish hue in the center to slightly cooler, bluer tones in the outer regions. There is some subtle evidence of a disk component, although not as distinct as a spiral. No strong signs of active star formation are immediately apparent, and no major tidal disturbances or ongoing mergers are observed. Minor disturbances can be seen in the galaxy. The galaxy appears moderately massive, given its size and luminosity profile.
