The galaxy presents a largely smooth, elliptical morphology. There is a dominant, centrally concentrated bulge component exhibiting a yellowish hue, indicative of an older stellar population. The galaxy appears generally rounded in shape, lacking prominent spiral arm structures or a defined disk. Minimal signs of ongoing star formation are apparent from the image alone, although regions of bluer light may be faintly visible. No major disturbances or signs of merging activity are readily discernible. Overall, the galaxy appears as a relatively quiescent system with characteristics consistent with an elliptical classification.
