The galaxy appears to be a disk galaxy, viewed at a moderate inclination. The central bulge is prominent and exhibits a yellowish-red hue, suggesting an older stellar population with relatively little ongoing star formation. The disk component surrounding the bulge displays a greenish tint, possibly indicating the presence of younger, hotter stars and ongoing star formation. The galaxy's overall shape is elliptical, likely due to the viewing angle. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy's features appear relatively smooth, with no distinct spiral arm structures easily discernible in this image. It is likely a galaxy with a mass on the higher end, but experiencing very low star formation currently.
