The galaxy presents a largely elliptical morphology, exhibiting a smooth, concentrated light profile. The central region displays a bright, diffuse yellowish glow, suggesting an older stellar population with minimal ongoing star formation. Moving outward from the core, the color shifts subtly towards redder hues. The overall form lacks any prominent spiral arm structures or significant dust lanes and the galaxy does not appear to be undergoing any major merging activity. There is little indication of a defined disk component. The radial light distribution fades gradually from the core, lacking sharp edges or breaks, reinforcing the impression of an elliptical galaxy. The galaxy is not perfectly spherical, with an intermediate roundness. There are hints of minor disturbances in the outer regions.
