The galaxy appears as an elliptical structure, exhibiting a smooth, diffuse morphology with a high degree of central concentration. The core region displays a yellow hue, likely indicating an older stellar population dominating the light output. Progressing outward from the core, the color gradually shifts towards a more greenish tint, perhaps suggesting the presence of a younger stellar population and/or some level of ongoing star formation, albeit relatively subdued. There's little evidence of spiral arm structures or significant dust lanes within the galaxy's disk, which points towards a relatively quiescent nature. The galaxy's overall shape appears generally well-defined, with no obvious signs of major tidal disturbances or ongoing mergers. However, there is some minor apparent irregularity that could point to minor gravitational interaction with another galaxy. The overall size is moderate.
