This galaxy exhibits a prominent central bulge with a smooth, elliptical appearance. The light is concentrated toward the center, gradually fading into a more diffuse halo. Faint spiral arm structures appear to emanate from the central region, though they are not tightly wound or clearly defined. The overall color is predominantly yellow-white, suggesting an older stellar population. There are subtle hints of blueish regions, possibly indicating areas of recent star formation, interspersed throughout the disk and outer regions of the galaxy. However, these regions are not particularly pronounced, supporting a classification leaning away from a strongly active star-forming galaxy. There is no indication of a major ongoing merger. There is a possible minor disturbance in the main galactic body, such as tidal tails or lopsidedness.
