The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. A concentrated central bulge is apparent, exhibiting a yellowish hue indicating an older stellar population. The outer regions of the galaxy gradually fade into the background, with little discernible structure or spiral arm features. A subtle bluer region is present on one edge of the galaxy. The overall shape approximates roundness, though a slight elongation cannot be ruled out. There is no visually significant evidence of ongoing major mergers or tidal disturbances. The relatively smooth appearance and color profile suggest a galaxy that has largely ceased active star formation in its central regions.
