The galaxy presents as a moderately inclined disk galaxy. A central bulge is visible, appearing relatively smooth. The disk exhibits subtle features, hinting at spiral arm structure, although they are not sharply defined. The color gradient suggests active star formation, with bluer hues concentrated within the disk and a redder tinge towards the bulge, possibly indicating an older stellar population in the galactic center. There are some minor disturbances to its morphology, possibly due to gravitational interactions with smaller galaxies or internal processes. Overall, the galaxy exhibits characteristics intermediate between a pure elliptical and a fully formed spiral, possibly reflecting an ongoing evolutionary process.
