The galaxy presents a generally smooth morphology, appearing elliptical in shape with a high degree of central concentration. The core region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. This color likely arises from the prevalence of red giant stars. Moving outward from the core, the color gradually shifts to a bluer tint, although no distinct spiral arm structures are observed. The faint blue halo suggests the presence of a younger population of stars in the outer regions. There are no obvious signs of recent major merger events, though some minor irregularities are apparent, suggesting possible tidal disturbances. The galaxy appears relatively isolated within its immediate environment. The galaxy appears to be undergoing relatively low levels of star formation.
