The galaxy presents as a relatively smooth, elliptical-like structure. There's a notable concentration of light towards the central region, suggesting a prominent bulge. The galaxy exhibits a generally round morphology with minimal visible disturbances or tidal features, indicating that it is likely not undergoing any major merging events. The color profile appears to be weighted towards the redder end of the spectrum, which could indicate an older stellar population and a lower rate of ongoing star formation. The overall appearance suggests a massive and relatively quiescent system.
