The galaxy appears to be elliptical in morphology, displaying a smooth, symmetrical light distribution without prominent spiral arms or a distinct disk. The galaxy exhibits a bright, concentrated core region that gradually fades into a diffuse halo. Color gradients are subtle, with a suggestion of slightly bluer hues in the outer regions compared to the yellowish-white core. The overall structure appears undisturbed, suggesting a lack of recent major merger events. There is no indication of significant dust lanes or active star formation regions within the observed area, consistent with an older stellar population. The galaxy's redshift suggests it is at a significant distance from the observer. The overall shape is close to round. 
