The galaxy presents as an elongated, disk-like structure oriented approximately edge-on relative to our line of sight. A central bulge is evident, appearing brighter and more compact than the surrounding disk. The disk exhibits a mottled appearance, with a mixture of brighter and fainter regions, potentially indicative of spiral arm structures, though the edge-on orientation makes these features difficult to definitively resolve. The color profile varies, with a bluer hue concentrated in the central region and a gradient towards redder tones extending outward from the nucleus. This suggests ongoing star formation activity in the core region. There is evidence of possible tidal features or minor disturbances present along the outer edges of the galaxy, possibly caused by a minor interaction with another galaxy. Based on these observed features, the object may be classified as a spiral or lenticular galaxy undergoing some type of minor interaction. Higher resolution imaging would be required for a more precise classification.
