The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population. Surrounding this core is a more diffuse, bluish halo. The halo appears relatively uniform in color and texture, suggesting a lack of significant recent star formation. There is no obvious spiral arm structure or prominent dust lanes visible within the galaxy. Overall, the galaxy's morphology suggests a relatively evolved system, potentially an elliptical or lenticular galaxy. Minor disturbance such as a small tidal tail cannot be ruled out due to the image quality.
