The galaxy presents as an elliptical morphology, with a smooth and largely featureless light distribution. It exhibits a slightly elongated shape, appearing somewhere between round and cigar-shaped, but trending more towards the rounded end. The central region is noticeably brighter, indicating a concentration of older stellar populations. 

There's a hint of a possible minor disturbance on one edge of the galaxy, presenting as a very faint and slightly bluer region, though it could also be an artifact of the imaging process. Overall, the galaxy does not show strong evidence of ongoing star formation, suggesting that its star formation activity is suppressed. It has an inferred large mass, approximately 10^11 solar masses. This galaxy appears to be a relatively evolved system, with a dominant smooth component.
