The galaxy presents a largely smooth and elliptical morphology. The core exhibits a high degree of luminosity, with a general color profile suggesting a population dominated by older stars. There is little to no apparent substructure, such as spiral arms or dust lanes, visible at this resolution. The galaxy's shape appears to be moderately flattened, exhibiting an axis ratio that deviates from perfectly circular. There are no signs of any significant tidal disturbances or ongoing merger activity in this image. A slight color gradient is observed, with the central regions appearing more yellow, potentially indicating a higher concentration of older stars, and bluer peripheries. Based on these characteristics, the galaxy can be classified as a relatively massive early-type galaxy, possibly an elliptical galaxy, at a redshift suggesting it is at an intermediate distance. The low rate of star formation is further consistent with an older stellar population.
