The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The light distribution suggests a high degree of radial symmetry. The central region exhibits a brighter, more concentrated luminosity, potentially indicating a higher density of stellar populations or the presence of an active galactic nucleus, though no distinct nucleus is discernible from this imagery. 

The colour profile appears relatively uniform across the galaxy, exhibiting a yellow-red hue. This suggests an older stellar population is dominant, which would be consistent with a low rate of star formation. There is no evidence of spiral arms, dust lanes, or significant ongoing star formation activity as indicated by the lack of blue emissions. The galaxy appears to be an isolated system with no signs of major tidal disturbances or ongoing mergers, though faint hints of minor irregularities cannot be ruled out. Overall, this galaxy presents the typical characteristics of an evolved elliptical galaxy.
