The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge that fades into a more diffuse halo. The color profile suggests a population dominated by older stars, with a notable absence of blue light indicative of recent or ongoing star formation. The galaxy appears to be generally undisturbed, showing no prominent signs of tidal features or major interactions that would suggest a recent merger. It is likely a massive system with a significant stellar mass.
