The galaxy appears to be a spiral galaxy, observed at an angle that presents it as elongated in shape. The central bulge is prominent and exhibits a yellowish hue, indicative of an older stellar population. Extending outwards from the bulge, faint bluish arms are discernible. These arms suggest ongoing star formation activity. There is no obvious active galactic nucleus or signs of strong interaction. The overall structure is relatively undisturbed, although there is slight irregularity noted in the outer disk. The galaxy seems to be relatively isolated in its environment.
