The galaxy presents as a predominantly smooth, elliptical structure, with a concentrated central bulge. There is a general lack of resolved spiral arm features. The galaxy exhibits a fairly homogenous yellowish-red color gradient moving from the core outwards, suggesting a primarily older stellar population. A slight asymmetry is potentially visible, with a hint of a disturbance on its left side. No strong indications of ongoing major merger events are apparent. The galaxy's overall shape is nearly circular, showing minimal elongation. The subdued star formation activity is implied from the color profile, with a dominant quiescent state.