The galaxy presents as an elongated, luminous object with a relatively smooth appearance. Its central region exhibits higher luminosity, suggesting a concentration of stars. The light distribution gradually decreases towards the outer edges, with some indication of a faint, extended disk. There is a slight blue tint to the galaxy overall, but this is most distinct toward the center. There is not much structure within the main body of the galaxy, with no distinct spiral arms. There also does seem to be some disturbance to the structure, suggesting the possibility of a past or current merging event.
