The galaxy presents as a single, moderately luminous object. Its morphology appears predominantly smooth and relatively round. There is a central concentration of light, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter light extends outwards from this core. The colour is indicative of a galaxy with a relatively low star formation rate. Evidence suggests that the galaxy is potentially undergoing a merging event with another galaxy, as suggested by the slightly disturbed, non-uniform structure.