The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. Its morphology is generally elliptical, appearing more 'in between' round and cigar shaped, rather than a highly flattened disk. There is an apparent central bulge that is slightly more yellow/red in color suggesting an older stellar population. The outer regions are bluer, indicating the presence of younger, hotter stars, although star formation is apparently limited. No significant spiral arm structures or dust lanes are readily discernible from the image. There is no strong indication of any major merging events or significant tidal disturbances impacting the galaxy's overall structure. The general appearance suggests a galaxy that has largely exhausted its gas supply and is undergoing a relatively quiescent period of star formation.
