This galaxy presents as an elongated structure, viewed nearly edge-on. It has a central bulge that appears yellowish in color, suggestive of an older stellar population. Surrounding the bulge is a disk, which exhibits a bluer hue, potentially indicating the presence of younger, hotter stars. The dust lane appears warped and distorted, perhaps due to gravitational interactions. Overall, the galaxy's morphology suggests it is a disk galaxy with a prominent bulge, exhibiting signs of possible disturbance or interaction.
