This galaxy appears as a relatively smooth object, exhibiting a predominantly elliptical morphology. The central region presents a high concentration of light, indicating a prominent nucleus or bulge. The galaxy displays a slight color gradient, with the core showing a more yellowish or reddish hue, potentially indicating an older stellar population. Moving outwards, the galaxy fades into a bluish halo, which is perhaps suggestive of some ongoing star formation, although it appears subdued. There is no indication of significant spiral arm structure or prominent dust lanes. The overall appearance suggests a galaxy with a considerable stellar mass, exhibiting a moderate level of star formation. There are hints of a possible minor disturbance in its structure, though this is not strongly apparent.
