The galaxy presents as a flattened, disk-like structure, viewed at a high inclination. The central region exhibits a concentrated, bright, yellowish-white hue, likely indicating an older stellar population within the galactic bulge. Moving outward from the center, the disk displays a subtle gradient toward bluer colors, possibly indicative of younger, hotter stars and ongoing star formation within the spiral arms. Faint, diffuse features are visible within the disk, hinting at spiral arm structures, although they are not sharply defined. The overall morphology suggests an elliptical galaxy with some star formation occurring. There appears to be very minor tidal disturbance visible in the structure. The light from this object suggests a moderately massive galaxy.
