The galaxy presents as an elliptical morphology. It has a notable bulge that transitions smoothly into the extended disk. The light distribution in the central bulge is concentrated and appears yellow-white, suggesting an older stellar population. Moving outward, the disk shows a bluer hue, indicating the presence of younger, hotter stars and some ongoing star formation. The galaxy's outline isn't perfectly smooth, there seems to be a disturbance along the edge of the galaxy, possibly signs of tidal interactions, but it is difficult to tell. There appears to be no distinct spiral arm structure. The galaxy's overall color index is shifted towards the red end of the spectrum, likely due to its intermediate redshift. The Petrosian radius extends a moderate distance from the center, showing a sizable galaxy. The galaxy is observed at an inclination, with the major axis oriented at roughly 140 degrees, suggesting a flattened shape. The galaxy is not extremely distant, yet it is far enough away that detailed features are somewhat blurred.
