The galaxy presents an overall elliptical morphology, though with a slight asymmetry, hinting at a possible disk component. The central region displays a concentrated luminosity with a yellow-orange hue, suggesting a population of older stars. Progressing outwards from the core, the colour shifts to a bluer tinge, particularly on one edge of the galaxy. This may be due to a region of relatively recent star formation. There is minimal evidence of spiral arm structure in the image. There are no obvious signs of a major ongoing merger event.
