This galaxy presents as a generally smooth, elliptical-like object, appearing quite round in shape. There is a concentrated central bulge that exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the center, the light becomes more diffuse, transitioning to a slightly bluer color, indicating the potential for some ongoing star formation, although limited. There is no discernible spiral structure or distinct features, giving the appearance of a relatively quiescent system. There seems to be no major signs of ongoing interaction or merging activity, though the possibility of minor disturbances cannot be completely ruled out due to the image resolution. Overall, the galaxy appears to be a fairly massive, well-established system with a mix of stellar populations.
