This galaxy appears to be a single, relatively smooth object with a central bulge. It is somewhat elliptical in shape, leaning towards being in-between a round and elliptical morphology, with a hint of a disk structure. There is evidence of star formation activity, particularly in the central region, inferred from its blueish hue and potential presence of HII regions. The overall color of the galaxy suggests an older stellar population, although some younger, bluer stars are present. The galaxy does not seem to be undergoing any major merger events, but there may be some minor disturbances present in its structure.
