The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated central bulge that is relatively bright and appears yellowish-orange in color. This core is surrounded by a more diffuse halo that fades gradually into the background. There are hints of faint blueish regions indicating the presence of some star formation, although the bulk of the galaxy seems to consist of an older stellar population. There does not appear to be any strong tidal features or obvious signs of recent major mergers, though subtle disturbances are potentially present, warranting further investigation. Overall, the galaxy appears to be a fairly massive system at moderate redshift, with a dominant spheroidal component and low levels of star formation. Higher resolution imaging and spectral analysis would be beneficial to more thoroughly assess morphological and stellar population characteristics.
