The galaxy presents as a relatively smooth, centralized light distribution with an elliptical morphology. There is a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. The outer regions show a subtle transition to a slightly bluer hue, hinting at the presence of younger stars, but this is not prominent. No distinct spiral arm structures or bar features are discernible. There is no significant dust lane obscuration or obvious tidal features indicating any major recent merger events. Overall, the galaxy appears to be a relatively undisturbed, early-type galaxy with ongoing, albeit low, star formation activity.
