The galaxy presents a generally smooth morphology, with minimal apparent substructure. The light profile indicates a concentrated central bulge that dominates the overall luminosity. The galaxy exhibits an elliptical shape, approaching a rounded form but with a slight elongation. The color profile is relatively uniform, with a subtle shift towards redder hues in the central regions. There's no visually discernible evidence of ongoing or recent major merger events, though minor disturbances cannot be ruled out at this resolution. Its relatively faint blue emissions suggest low star formation. This object is likely a mature galaxy with a substantial stellar mass.
