The galaxy appears as an elliptical or lenticular type galaxy, exhibiting a primarily smooth morphology, but potentially harboring faint disk-like features. There is an absence of well-defined spiral arms. The light distribution suggests a centrally concentrated spheroid shape with moderate ellipticity. The color profile indicates a generally older stellar population, skewed towards redder wavelengths.

There's suggestion of minor gravitational disturbance or tidal interaction based on slight asymmetry of light, but galaxy seems relatively unperturbed. Overall, the galaxy appears to be a relatively massive system with suppressed star formation activity, suggesting an evolved and passive state.
