The galaxy appears as a single, concentrated light source, with an elliptical morphology based on the images provided. A dominant yellow color is present in the galaxy's central region, which becomes slightly redder towards the periphery. The central region appears smooth with no apparent substructure. The overall appearance suggests a lack of significant spiral arms or a prominent disk-like structure, indicative of an older stellar population with minimal recent star formation activity. There are no indications of any ongoing major merging events or tidal disturbances.
