The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core region exhibits a bright, yellowish-white luminosity, suggesting an older stellar population. Progressing outwards from the center, there is a gradual decrease in surface brightness. The overall shape appears to be moderately elongated, with the major axis extending horizontally across the image. Faint blue hues can be observed, indicating regions of some recent, albeit low, star formation activity. There does not appear to be evidence of significant disturbances or ongoing major mergers. The galaxy lacks distinct spiral arm structures or a prominent disk.
