The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively featureless. A centrally concentrated bulge is prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Surrounding the bulge is a more diffuse region, showing a bluer color, potentially indicating ongoing or recent star formation. There is evidence of some minor disturbances or irregularities in the outer regions of the galaxy, possibly indicative of past interactions or mergers. There is a hint of a faint disk-like structure, but it is not well-defined. The galaxy exhibits a moderate redshift, suggesting it is at a considerable cosmological distance. Based on color, the galaxy has moderate amounts of star formation. The galaxy appears to be quite massive, with a substantial stellar population.
