The galaxy presents a generally smooth, elliptical morphology. Its light profile indicates a fairly concentrated central bulge, with the intensity gradually decreasing outwards. Color analysis suggests the presence of older stellar populations, as it appears relatively red. There is no discernable disk structure or spiral arms visible within the galaxy. There is no evidence of significant ongoing star formation from what I can observe. Its overall shape appears rounded, without any significant disturbances or tidal features that would suggest a recent major merger event. The galaxy is relatively compact in size. 
