The galaxy appears as a centrally concentrated object with a generally smooth morphology, exhibiting a nearly circular profile. The light distribution suggests a dominant bulge component. There is a faint hint of some possible irregular structure extending outward, perhaps a very faint, disturbed disk. The galaxy displays a color gradient, with a more yellowish-white core and a slightly redder outer halo. There is no clear evidence of spiral arms or significant dust lanes within the resolution of the image. The galaxy appears relatively isolated.
