The galaxy appears to be a spiral galaxy, viewed nearly edge-on. There is a prominent central bulge with a yellow-white hue, suggesting an older stellar population dominating the core. The disk is elongated and relatively smooth in appearance, with a faint bluish tinge along the edges, indicating the presence of younger, hotter stars and possible ongoing star formation. The disk exhibits some signs of minor disturbances. There is no clear evidence of a major merger or significant tidal interactions with neighboring galaxies. Dust lanes are not distinctly visible, but the subtle color variations and slight irregularities in the disk's light distribution hints at their presence. The galaxy displays a moderate level of star formation activity. Its estimated size suggests it is a dwarf galaxy.
