The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that is bright and yellowish in color, suggesting an older stellar population. The galaxy's overall shape is generally round, with only a slight deviation from perfect circularity. There is no distinct disk structure or spiral arm features visible. No signs of any major ongoing merging or tidal disturbances are present. Faint outer regions of the galaxy appear to dissipate smoothly into the background sky, lacking defined edges. The lack of blue color suggests a low rate of ongoing star formation.
