This galaxy exhibits an elliptical morphology, with a predominantly smooth, centralized structure. The core region displays a concentrated luminosity gradient, suggesting a higher stellar density. Radially outward, the light gradually diffuses into a fainter, less defined halo. The galaxy appears somewhat rounded in shape, showing a slight deviation from a perfectly circular form. There is no apparent evidence of prominent spiral arms or a distinct disk structure. A faint blue tinge around the outer halo indicates the presence of a younger stellar population or ongoing star formation, although the overall color suggests an older, redder stellar population dominates the galaxy. There are no signs of significant tidal disturbances or ongoing merger activity in this image, although subtle distortions in the outer isophotes cannot be entirely ruled out.
