This galaxy presents as a relatively smooth, elliptical-like structure with a distinct central bulge. The overall color appears to be skewed towards the red end of the spectrum, suggesting an older stellar population. The galaxy's shape is somewhat elongated, but not dramatically so, tending towards a moderate ellipticity. There is no obvious spiral arm structure or significant dust lane visible, indicating it may be a lenticular or elliptical type galaxy. No major disturbances or mergers are evident in the current image, though minor asymmetries cannot be ruled out at this resolution. The light is concentrated with a smooth profile, lacking the clumpy or irregular features often associated with intense star formation regions. The overall impression is of a galaxy in a relatively quiescent state, past its peak star-forming epoch.
