The galaxy presents as a predominantly smooth, elliptical-like structure with a high degree of central concentration. Its morphology indicates a relatively evolved system. The color profile suggests a higher proportion of older stellar populations, particularly concentrated towards the core, which displays a yellowish hue. There's a slight asymmetry in the outer regions, hinting at a possible minor disturbance, merger event, or tidal interaction. The galaxy exhibits a relatively compact size, suggesting a moderate physical extent. The overall light distribution is consistent with a galaxy undergoing a period of relatively low star formation activity.
