The galaxy exhibits a generally smooth morphology, appearing largely featureless. It displays a slightly elongated, elliptical shape. A central bulge region is visible, exhibiting a concentrated luminosity with a yellow-orange hue, indicative of an older stellar population. The galaxy's overall color suggests a relatively passive star formation rate. The outer regions present a gradual fading in luminosity, with no distinct spiral arms or strong tidal features. The observed morphology indicates the galaxy is likely an early-type galaxy, potentially an elliptical or lenticular type, with minimal signs of recent merger activity or significant star formation in the disk.
