The galaxy presents as a relatively smooth, centralized object. Its overall form appears elliptical with a slight deviation from perfect circularity. The color profile suggests an older stellar population, with a dominant yellow-red hue concentrated in the central bulge. There is a subtle hint of bluer colors at the edges suggesting a degree of on-going star formation but this activity is not dominant. There are no prominent spiral arms, bars, or other disk-like features visible, indicating a generally spheroidal morphology. No obvious signs of active galactic nuclei are seen, and there is no strong evidence of any major ongoing merging events or tidal distortions. Faint perturbations or minor disturbances may be present, but they are not prominent.
