The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated, bright central bulge, suggesting a high stellar density in the core region. The galaxy's overall shape is largely spheroidal. There is a slight deviation from perfect circularity, with the galaxy exhibiting a mild ellipticity. The color profile suggests an older stellar population. The core region displays a yellowish to orange hue, characteristic of evolved stars. Moving outward from the center, the color gradually shifts toward redder tones, indicating a dominance of older, cooler stars in the outer regions. There are no prominent spiral arms, dust lanes, or other distinct features typically associated with spiral galaxies, leading to the assumption that star formation is not occurring at a high rate. No signs of major mergers or tidal disturbances are evident in the image.
