This galaxy presents as a disk galaxy, viewed at an angle that is slightly off from edge-on but not quite face-on. The central bulge appears prominent, contributing significantly to the galaxy's overall luminosity. Faint spiral arm structures may be present, although this is difficult to confirm due to the apparent smoothing of the image. There may also be the presence of a bar-like structure running through the center of the galaxy.

The color distribution suggests an older stellar population in the bulge, indicated by its yellowish-orange hue. Some bluer regions, possibly indicative of ongoing or recent star formation, are seen in the outer disk.

The elliptical shape of the galaxy suggests a disk morphology with an axis ratio of approximately 0.6. The object has an estimated radius of roughly 4 kpc.
