The galaxy presents as a somewhat asymmetrical, moderately luminous structure. It appears largely smooth with a slightly elongated morphology, lacking prominent spiral arm features. The central region exhibits a concentrated, bright core, suggesting the presence of a significant stellar population or an active galactic nucleus. A subtle color gradient is observable, with the core showing a yellower hue, potentially indicative of older stellar populations, while the outer regions exhibit a bluer tint, which could point to more recent star formation activity. There is a slight hint of a possible disturbance or interaction visible in the upper portion of the galaxy, suggestive of a minor gravitational interaction with another galaxy. Overall, the galaxy appears to be a relatively massive system with a mixture of stellar populations and an ongoing, albeit perhaps subdued, rate of star formation.
