The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that graduates to a more diffuse halo. The core exhibits a yellowish-orange hue, suggesting a population of older, redder stars. Progressing outward, the surrounding region becomes more blue, hinting at regions of more recent star formation, albeit not as prominent or defined as in spiral galaxies. The overall shape is largely round. There is no obvious evidence of tidal tails, distorted morphology, or ongoing mergers. The light distribution is relatively uniform without strong indicators of spiral arms or prominent dust lanes.
