The galaxy appears as a relatively compact object at a redshift of approximately 0.15. Its morphology suggests a possible ongoing merger or interaction. One core of the galaxy is smooth and features a yellowish-white hue, possibly indicative of an older stellar population or dust obscuration. Adjacent to this is a less defined region exhibiting a bluer and more mottled appearance, suggestive of active star formation. The overall shape of the system is elongated, with a general lack of defined spiral structure, leaning towards a more irregular or peculiar classification. There is some evidence of tidal features or disturbances, though the low resolution makes them difficult to definitively resolve. The galaxy exhibits a moderate level of star formation activity. The estimated size of the galaxy is roughly 4 kpc in radius.
