The galaxy presents a predominantly edge-on disk morphology. The disk appears elongated with an approximate major axis spanning approximately 3 arcseconds. There's a slight indication of a central bulge, characterized by a smooth and diffuse light distribution, transitioning into the disk. The disk shows evidence of internal structure, though not distinctly resolved. A possible merging companion or minor tidal disturbance is indicated by a faint asymmetry. The galactic nucleus is compact and is a central point of bluer light. The disk exhibits a general color gradient from a bluer central region to redder outer edges. The overall color suggests the possibility of on-going star formation. The light distribution appears relatively smooth, without prominent spiral arms, suggesting a somewhat evolved spiral or a lenticular galaxy.
