This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. It displays a concentrated central bulge with a yellowish-orange hue, suggesting an older stellar population. The galaxy exhibits a moderate level of light concentration, with the intensity decreasing gradually from the center outwards. There are slight indications of a faint, extended halo surrounding the central region of the galaxy. This object presents with a redshift measured at approximately 0.13, indicating a considerable distance. There is no visible evidence of spiral arms, a prominent disk, or significant dust lanes. Based on the observed color gradient, we can infer a possible cessation of major star formation in the recent past. There are also some irregular features and asymmetric structures, which could imply past merger events.
