The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core region displays a bright, almost stellar-like nucleus, which fades into a more diffuse halo. A slight elongation is visible, deviating from a perfectly circular morphology. Color gradients are subtle, but a bluer tinge seems to be present in the outer regions of the galaxy, contrasting with the yellower central bulge. There is no clear evidence of spiral arms, bars, or prominent dust lanes. The galaxy does not appear to be significantly interacting with any other large objects. The overall impression is of a galaxy dominated by an older stellar population, but possibly with some ongoing, low-level star formation in its outer regions.
