The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. Its form is roughly elliptical, exhibiting a degree of roundness. A bright central bulge is prominent, surrounded by a fainter, more diffuse halo. The galaxy displays a color gradient, with the central region appearing slightly yellower than the outer regions, suggesting a population of older stars concentrated toward the core. There are subtle hints of bluer regions within the halo, potentially indicating areas of more recent star formation. No significant signs of major mergers or tidal disturbances are immediately apparent from this view, though subtle asymmetries might indicate minor interactions or internal dynamics. Based on its apparent magnitude and redshift, this galaxy is likely a luminous and massive system.
