The galaxy presents as a relatively smooth, centrally concentrated object. It appears moderately elliptical, showing more of an in-between profile than being perfectly round. There is some indication of a disk-like structure, but this is not a prominent feature. The galaxy exhibits a yellow-red hue, suggesting a population of older stars, but with some possible on going star formation. There's no strong evidence of a major ongoing merger, but some minor disturbance may be present in the galaxy's overall structure. It shows an estimated radius of 7.6 kpc based on half of the light, suggesting it's a moderately sized galaxy.
