The galaxy exhibits a generally elliptical morphology, appearing as a flattened spheroid. Its light distribution is relatively smooth, with a gradual decrease in surface brightness from the center towards the outer regions. The central region displays a yellowish hue, suggesting a higher concentration of older stellar populations. The outer regions show a bluer color, indicating the presence of younger, hotter stars. The shape of the galaxy is elongated, hinting at possible rotational flattening. There is a small, blue, circular object very close to the disk. The galaxy is relatively isolated. There are no other notable features visible within or immediately surrounding the galaxy.
