The galaxy presents an overall elliptical morphology, appearing largely smooth with a dominant central bulge. There is a slight elongation, but it is predominantly round in shape. The core exhibits a higher concentration of light, with a diffuse halo extending outwards. The galaxy exhibits an overall redder color, suggesting a population of older stars and a cessation of significant star formation. There is evidence of a possible ongoing or recent merger event, seen in the tidal-like features and irregularities within the galaxy's shape. While exhibiting characteristics of an early-type galaxy, the morphology indicates it is not a simple and undisturbed system.
