The galaxy presents a generally smooth and rounded morphology, with a centrally concentrated light profile. The shape appears to be somewhere between perfectly round and slightly elongated, with no obvious bar or spiral arm structures visible. There is a relatively subtle color gradient, transitioning from redder hues in the central regions to bluer tones toward the outer edges. The galaxy exhibits a moderately high redshift, placing it at a significant cosmological distance, thus its measured absolute magnitudes are quite high.

Based on estimated star formation rates, the galaxy is likely experiencing a relatively low level of star formation activity. The color gradient also supports this, given the presence of redder, older stellar populations in the core. The mass of the galaxy is significant, suggesting that it is a fairly substantial system, though not exceedingly massive. Minor disturbances may be present based on morphological classification, and may be in the process of a relatively minor merger event.
