The galaxy presents as a slightly elongated, elliptical-type galaxy with a smooth, diffuse appearance, possibly viewed at a non-negligible inclination. It exhibits a core region of concentrated light, diminishing gradually outward. There's a hint of asymmetry in its structure, with a potential, subtle disturbance or minor feature visible. The galaxy’s color profile leans toward redder wavelengths, suggesting an older stellar population and a comparatively quiescent star formation rate. The morphology indicates it has likely not experienced any major recent merging events.
