This galaxy exhibits a predominantly smooth morphology. The central region is characterized by a concentrated, bright core, suggestive of a significant stellar population. The light distribution appears nearly round, with a gradual decrease in intensity moving outwards from the core. There is a subtle color gradient, with the core appearing more yellow/orange, transitioning to bluer hues in the outer regions. This could indicate a difference in stellar populations, with older stars concentrated in the core and younger stars residing in the outer regions. I do not observe any clear evidence of spiral arms or a distinct disk structure, supporting its classification as a galaxy with a smooth appearance. Faint disturbances could be present within the system, however more data is required to come to a full conclusion.
