The galaxy presents as a relatively compact, elliptical-like object. It appears to be quite smooth, with a high degree of central concentration. There is a bright, yellowish core, potentially indicative of an older stellar population or an active galactic nucleus, with a red shift indicating its distance. The outer regions exhibit a more diffuse, slightly greenish/bluish halo, possibly indicating the presence of some younger, bluer stars, even though the overall star formation rate is probably low. The lack of distinct spiral arms or a well-defined disk structure suggests a morphological classification leaning toward an elliptical or lenticular galaxy, with some evidence of minor disturbance possibly due to past mergers. It does not present with a highly elongated shape, which would further corroborate its elliptical classification.
