The galaxy presents as a moderately luminous object with an overall bluish-white hue, indicative of a population of younger, hotter stars. Its morphology appears to be somewhat irregular, possibly a disk galaxy with a prominent central bulge. There is a hint of some spiral arm structure or disrupted features extending outward from the central region. The object exhibits no clear evidence of a dominant, well-defined structure, suggesting potential disturbances or interactions. There is a faint reddish area on one side of the galaxy, possibly a star forming region.
