The galaxy presents an elongated, cigar-shaped morphology. A distinct central bulge is not readily apparent, suggesting it could be a disk galaxy viewed edge-on, or potentially an elliptical galaxy. The color gradient indicates a redder hue towards the central region, possibly indicative of an older stellar population or higher dust concentration. The outer regions display bluer tones, hinting at younger stars or active star formation. There are no obvious spiral arm structures or bar features visible in this image. There may be minor distortions in the morphology, implying a possible past or ongoing interaction with another galaxy. The relative smoothness of the light distribution suggests that it is either a disk galaxy with minimal star formation or it has a considerable age. Its overall mass appears to be substantial. The rate of star formation is comparatively low for a galaxy of its size.
