The observed galaxy presents a flattened, disk-like morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a bulge component, likely containing an older stellar population. The disk itself appears to be viewed edge-on or nearly edge-on. A dust lane is clearly visible bisecting the galaxy along its major axis, absorbing light from the stars behind it and giving it the dark red coloring. There are some hints of possible tidal features or minor disturbances in the disk, perhaps indicating an interaction or merger event in its past. The galaxy displays a range of colors across its body, with yellower hues in the central regions and bluer tints within the disk, possibly indicative of ongoing star formation regions. Overall, this appears to be a spiral or lenticular galaxy undergoing some form of evolutionary process.
