The galaxy presents as a relatively compact system. Its overall morphology is elongated, suggesting a flattened shape viewed at an oblique angle, possibly a disk galaxy. The light distribution is concentrated toward the center, but appears more uneven than spheroidal, showing some irregular texture.

Color gradients are apparent, indicating variations in stellar populations or dust obscuration across the galaxy. The central region exhibits a warmer hue, potentially indicative of older stellar populations or dust extinction. Fainter bluer regions are present towards the outer areas of the galaxy, which may imply ongoing star formation activity. These regions lack well-defined spiral arm structures.

The galaxy displays some signs of tidal features or disturbances, such as a slight asymmetry in its outer regions and evidence of disruption in the general light distribution. This could indicate a past or ongoing interaction with another galaxy.
