The galaxy appears as a highly elongated, smooth object with a notable absence of distinct spiral arms. Its color profile indicates a predominantly older stellar population, with a redder hue concentrated at the core, and a fading blueish hue towards the outer edge. The central region of the galaxy exhibits high luminosity, decreasing gradually toward the edges. A dust lane is visible across the central region of the disk, giving the galaxy a clear line across its width. The overall shape suggests that this is an elliptical or lenticular galaxy, possibly seen edge-on. There are some very small pockets of bluer light, indicating that there may be areas of ongoing star formation, though at a very low rate. The apparent lack of disturbance in its morphology suggests a relatively isolated existence and that this galaxy is not currently undergoing any significant merger activity.
