The galaxy presents a generally smooth, elliptical morphology, though it does display some subtle features. The light distribution is centrally concentrated with a gradual decline in brightness toward the outer regions. There is a slight elongation to the galaxy's shape, appearing more disc-like but not overtly spiral. Color gradients are minimal, with the central region appearing slightly more yellow-white, while the outer regions are a bit fainter. There is no clear evidence of distinct spiral arms or prominent dust lanes. Based on its appearance and estimated redshift, this galaxy likely exhibits ongoing star formation. However, no intense bursts of activity are indicated by strong emission of light in the blue spectrum. There is a suggestion of some merging or tidal disturbance, based on some subtle irregularities and features. Overall, the galaxy seems to be in a relatively evolved state.
