The galaxy presents a primarily smooth morphology, with a central bulge that appears bright and concentrated. There is a faint disk-like structure surrounding the bulge, though it is not sharply defined, presenting a hazy, indistinct quality. Overall, the galaxy exhibits a slight blue tinge, suggesting moderate levels of recent or ongoing star formation. There is no clear evidence of strong spiral arm structures or bar features. The galaxy's overall shape appears elliptical but not perfectly symmetrical, indicating some level of internal dynamics or past interactions that could have disrupted its ideal smooth shape. There are no apparent tidal tails or other indicators of a major ongoing merger. Minor disturbances are not ruled out.
