The galaxy presents as an elliptical or lenticular structure with a smooth, diffuse light distribution, indicating a relatively evolved stellar population. A bright central bulge is prominent, surrounded by a fainter, more extended disk or halo. There is a slight bluing in the outer regions, which suggests some ongoing star formation, albeit at a low rate. Overall, the galaxy does not exhibit any signs of significant morphological disturbance, suggesting it is relatively undisturbed by recent major merger events. Subtle asymmetries may indicate minor disturbances, but the galaxy appears largely settled in its structure.
