The galaxy presents as a relatively smooth, elliptical or lenticular structure. It appears moderately rounded, showing a slight departure from a perfectly circular form. The central bulge is prominent, exhibiting a concentrated and bright luminosity. The surrounding disk or halo region displays a bluer hue, suggesting the presence of younger stellar populations and ongoing star formation, although at a moderate rate. There is no strong evidence of significant tidal disturbances or major ongoing mergers. The morphology is largely undisturbed, with only subtle signs of minor interactions or internal activity. The galaxy displays a red shift, indicating that it is at a considerable distance from our own, but it is still possible to determine that it is relatively massive.
