This galaxy presents as a moderately sized, somewhat diffuse object. The central region exhibits a brighter, more concentrated luminosity, suggesting a galactic bulge or nucleus. The overall shape appears somewhat irregular, possibly exhibiting a disk-like structure viewed at an angle. There is a faint blue hue apparent, particularly within the more diffuse regions, hinting at the presence of younger, hotter stars and ongoing star formation, but at a relatively low rate. Some indications of minor disturbances are seen, with slight asymmetries and hints of tidal features or interactions. There doesn't appear to be any dominant spiral arms. It is likely to be a galaxy with an intermediate stellar mass.
