The galaxy appears to be a somewhat elliptical, disk-like structure, displaying a smooth overall morphology. Its shape is elongated, tending toward a cigar shape. A notable feature is its color gradient, shifting from a central, yellowish-orange hue to fainter, greenish-blue fringes at its periphery. This suggests a difference in stellar populations or dust content between the core and outer regions. The primary body exhibits a relatively smooth texture, hinting at a lack of significant, ongoing mergers or major disturbances despite faint signs of disturbances. There is no discernible spiral arm structure. The galaxy’s overall light profile seems well-defined but diffuse, indicating substantial mass content and relatively active star formation at an estimated distance.
