The galaxy exhibits a predominantly smooth morphology, with a slightly elliptical shape that is more in between elliptical and round. The central region is significantly brighter and more concentrated than the outer regions, suggesting a prominent galactic bulge. There is a slight suggestion of a disk or spiral arm structure in the outer regions, with a hint of structure, but it is not very defined. The galaxy displays a colour gradient, with the central bulge appearing more yellow/orange, which is indicative of an older stellar population. The outer regions show bluer hues, possibly due to the presence of younger stars. There is no obvious evidence of significant recent merging activity, or major disturbances within the system, and the image does not show any clear signs of ongoing, high-intensity star formation regions. The galaxy is a relatively massive system, as can be inferred from its overall luminosity.
