The galaxy presents an elliptical morphology, exhibiting a smooth and somewhat diffuse appearance. Its core region displays a concentrated, yellowish hue, indicating a likely older stellar population. The outer regions appear less defined, fading gradually into the background. There is a subtle blue tint around the edges, possibly indicating regions of more recent, albeit limited, star formation activity. The overall shape is noticeably elongated, though not extremely so, suggesting a moderate degree of flattening. There are no clear signs of major disturbances or merging events, though the possibility of minor interactions cannot be ruled out based on the image alone.
