The galaxy appears as a relatively smooth, elliptical object, exhibiting a primarily yellowish-orange hue, suggestive of an older stellar population and lower levels of active star formation. The morphology indicates a somewhat rounded shape, leaning towards elliptical rather than a highly elongated structure. There is no clear evidence of a prominent disk component, spiral arms, or significant dust lanes within the galaxy. The light distribution seems concentrated towards the center, with a gradual fading towards the outer regions, forming a somewhat diffuse halo. The galaxy does not appear to be undergoing any major merging events, although some minor disturbances cannot be entirely ruled out based on the image alone.
