This galaxy presents as a slightly elongated, elliptical structure with a bright, concentrated central bulge. The color gradient suggests the presence of an older stellar population within the core, indicated by the yellowish-white hue. Moving outwards from the core, the galaxy exhibits a less concentrated disk, with subtle hints of bluer regions, potentially indicative of more recent star formation. Overall, the galaxy appears relatively smooth with a minimal amount of disturbance. It does not display any prominent spiral arms or a bar structure. It is plausibly undergoing a very minor merger or disturbance event, but is generally relaxed and unperturbed.
