The galaxy presents as a relatively smooth, centrally concentrated elliptical system. The light profile appears largely featureless, lacking defined spiral arms or a prominent bar structure. The core exhibits a bright, concentrated luminosity suggesting a significant stellar population and possibly an active galactic nucleus. The overall shape appears nearly round, exhibiting minimal elongation or asymmetry. There is a slight color gradient observed, with the central region appearing more yellowish/white, transitioning to slightly redder hues in the outer regions. These colors indicate an older stellar population. Minor disturbances or merging features are not clearly discernible, suggesting a dynamically relaxed system. Star formation is likely occurring at a moderate rate. The galaxy appears to be an isolated system.
