The galaxy presents as a relatively small object. Its central region exhibits a smooth appearance, with a yellowish-white hue, possibly indicating an older stellar population. Emanating from this core is what looks to be a flattened disk, which is slightly more extended along one axis than the other, hinting at a possible disklike structure.

There are indications of some structure within the disk, although it is not clearly resolved. A faint blueish tint to one side of the disk suggests the possibility of younger stars, perhaps indicating ongoing star formation. The overall morphology doesn't seem particularly disturbed, with only minor possible distortions. There appears to be no significant signs of an active merger.