This galaxy appears to be a relatively smooth, single object. The light is concentrated in the center, with a gradual decrease in brightness towards the edges. The central region exhibits a yellowish color, suggestive of an older stellar population. Fainter, bluer regions can be observed along the periphery, indicating the presence of some younger, hotter stars, and/or areas of active star formation, although limited. There is some asymmetry observed in the outer light distribution, which may possibly imply tidal interactions, but this is not certain based on this image alone. The galaxy does not appear to be a classic spiral or barred spiral, but more likely an elliptical type or a lenticular galaxy with a dominant bulge. The apparent size is relatively small, which, in combination with its redshift, means that this galaxy is likely to be quite luminous and massive. 
