The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The shape appears elongated, deviating noticeably from a circular form. The color gradient suggests a relatively homogenous stellar population, with a subtle shift towards redder hues in the central bulge. There is no prominent disk structure or spiral arm features visible. Faint asymmetrical disturbances can be noticed at the edges of the galaxy. The overall appearance indicates an evolved system, potentially undergoing minor interaction with smaller galaxies in the vicinity.
