The galaxy presents as a somewhat irregular object. It is characterized by a central, relatively smooth region that may represent a bulge or a dense concentration of older stars. Surrounding this central region are more diffuse, less defined structures with hints of blue coloration, suggesting the presence of younger, hotter stars, possibly indicating ongoing star formation. There also appears to be disturbed features, possibly resulting from an interaction or merger with another galaxy. These disturbances manifest as asymmetric extensions or tidal features that deviate from a regular elliptical or spiral shape. Overall, the galaxy shows a mixture of smooth and irregular components, possibly suggestive of an ongoing merger event that is stirring up the star formation within the object.
