This galaxy appears to be a disk galaxy viewed at an oblique angle. The central bulge is prominent and relatively bright, exhibiting a yellowish-white hue, suggesting an older stellar population with less active star formation in that region. The disk itself is visible, extending outwards from the bulge. Within the disk, a hint of bluer colors can be observed, possibly indicating the presence of younger, hotter stars and ongoing star formation, even if at a modest rate. The galaxy has a somewhat elongated shape, more lenticular than spiral, with no obvious arm structure or major disturbances evident. The overall morphology seems relatively smooth, with a fairly symmetrical distribution of light.
