The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. The dominant color is a yellowish-white, indicative of a stellar population dominated by older, evolved stars. There is a subtle hint of a slight flattening or elongation, but the overall shape appears relatively round. No distinct spiral arm structures or prominent dust lanes are discernible. There is some suggestion of minor disturbances to the shape, such as a slight tidal tail, but its general structure would suggest it has no merger. The galaxy's color suggests that there is very low star formation, a typical attribute of older stellar populations.
