The object presents as a galaxy with a relatively compact form. The galaxy exhibits a disk-like structure, oriented approximately edge-on from our vantage point. There is a notable central bulge that appears to be a brighter, more concentrated region. The color distribution suggests the presence of older stellar populations within the bulge, as indicated by its redder hue, while bluer colors are concentrated in the disk, suggesting ongoing or recent star formation. Faint tidal features may be present, suggesting past or ongoing interactions with another galaxy, or perhaps simply due to internal disturbances. The main body of the galaxy appears disturbed, with some evidence of tidal tails or other features.
