The galaxy appears as an amorphous, moderately bright structure. There is a notable lack of defined spiral arms or a prominent central bulge. The light distribution is somewhat irregular, with hints of tidal features or distorted morphology, suggestive of gravitational interaction with another galaxy. There are several distinct clumps of brighter luminosity scattered throughout the galaxy which could be indicative of active star formation regions. The color profile appears somewhat redder overall, suggesting a population of older stars and/or significant dust obscuration.
