The galaxy presents an elongated morphology, appearing approximately 8 kpc in its major axis. The light distribution is not uniform, exhibiting two distinct regions of enhanced emission. The primary concentration of light is located in the center of the galaxy, which has a yellowish hue. This central region appears relatively smooth and lacks well-defined spiral arm structures. A secondary concentration of light is located towards the bottom of the galaxy, appearing blue in color. This likely indicates recent star formation. The overall morphology suggests a galaxy experiencing some form of disturbance or interaction, possibly undergoing a minor merger. There are no clear tidal tails or other prominent features indicative of a major ongoing merger, but the presence of an asymmetrical light distribution suggests that gravitational interactions have played a role in shaping the galaxy's present appearance.
