The galaxy appears as a relatively compact, luminous structure. The object exhibits a generally elliptical morphology, with a high degree of central concentration. There are two bright, diffuse regions within the galaxy's envelope. These regions might be the result of merging galaxies. The overall color is suggestive of an older stellar population. The object seems relatively isolated and undisturbed beyond minor gravitational disturbances. There is no clear evidence of distinct spiral arms or a prominent disk structure. Given the observed morphology and colour, the galaxy may be an early-type galaxy undergoing a merger.
