The galaxy appears as a centrally concentrated object, exhibiting a smooth and generally elliptical morphology. A bright, yellowish core dominates the galaxy's luminosity profile, suggesting an older stellar population within the galactic nucleus. Progressing outwards from the core, the light transitions into a less intensely luminous, more diffuse halo region. This outer halo displays hints of bluer hues, potentially indicative of a younger, albeit sparse, stellar population or regions of low-level star formation. There are no readily discernible spiral arm structures or significant dust lanes visible within the image. The overall form suggests the galaxy is likely a relatively massive system with a moderate amount of ongoing star formation relative to its stellar mass. There may be minor disturbances or interactions occurring, given slight asymmetries and irregularities in the outer halo, but overall it presents as a relatively isolated system in a late stage of its evolution.
