The galaxy presents as a slightly elongated, diffuse object with a smooth morphology. Its central region exhibits a brighter, more concentrated luminosity, suggesting a possible core or bulge. The overall color profile appears to be predominantly yellow-red, indicating a population of older stars. Faint hints of disruption are visible in the outer regions, possibly due to gravitational interaction with another galaxy in the past. The object's roundness is fairly typical for a galaxy and does not stand out. There are some hints of interaction, however they are minor and non-descript, making it difficult to definitively characterize without further data. The smoothness of the galaxy indicates a well-mixed stellar population with little recent major star formation.
