The galaxy presents an overall lenticular or disk-like morphology, viewed nearly edge-on. The central region appears as a bright, concentrated bulge that transitions smoothly into a fainter surrounding disk. Within the disk, there appears to be some irregular structure, potentially indicating the presence of dust lanes or spiral arm segments. There is a color gradient visible, with the central bulge exhibiting a slightly redder hue compared to the bluer light emitted from the disk. This may reflect differences in stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars populating the disk.
