The galaxy appears to be a disk galaxy, viewed nearly edge-on. A central bulge is prominent, exhibiting a concentrated yellowish-white luminosity, possibly indicating an older stellar population with reduced star formation activity. A relatively thin and faint disk extends outwards from the bulge. Within the disk, a subtle reddish hue can be observed, possibly indicating regions of dust obscuration or the presence of older stars. There are no apparent signs of strong spiral arm structure or active star forming regions. It seems generally smooth, but with some faint indication of possible disturbance or a slight asymmetry.
