The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The central region presents a concentrated luminosity, suggesting a prominent galactic nucleus. There is a color gradient with the central region exhibiting a yellow-red hue, potentially indicating an older stellar population, while the outer regions are slightly bluer in color, which could denote ongoing, albeit low levels of star formation. There is no obvious evidence of spiral arms or a disk-like structure. There are also no clear signs of any major mergers or strong gravitational disturbances.
