The galaxy appears to be a spiral galaxy seen at an oblique angle, close to edge-on but with some disc visible. A central bulge is prominent, exhibiting a yellowish hue which suggests an older stellar population. Fainter, bluish regions are observed along the outer edges of the disk, potentially indicating areas of ongoing star formation within spiral arms. The disk exhibits some irregularities and disturbances, hinting at possible past or ongoing gravitational interactions, but generally maintains a well-defined shape. There is no obvious sign of merging with any other galaxies.
