The galaxy appears to be a disk galaxy, viewed at a significant angle, approaching edge-on. The central bulge is prominent and displays a yellowish hue, indicative of an older stellar population. Extending from the central bulge is a faint disk structure, possibly exhibiting spiral arm features, though the resolution limits detailed observation. The color of the disk is bluer than the bulge, possibly due to ongoing star formation. There are no apparent signs of a major ongoing merger, however, there are signs of minor disturbances. The galaxy's overall shape is elongated, appearing somewhat cigar-shaped. There is some visual evidence to suggest the existence of dust lanes within the galaxy.
