The galaxy presents as a luminous, though somewhat ill-defined, structure. Its overall form appears irregular, showing no clear spiral arms or bar. The light distribution is uneven, with a brighter, more concentrated core and a fainter, diffuse halo or outer region. The object displays an orange-red hue, indicating a population of older stars and a relatively low rate of ongoing star formation. There is also a prominent second region of similar color and brightness that appears to be connected to the galaxy, which likely means the galaxy is undergoing a merger, or has just experienced a merger. The galaxy appears to be of considerable mass and luminosity given its distance. Overall, the object's morphology suggests it may be an elliptical galaxy, or an irregular galaxy undergoing a merger.
