The galaxy presents as a relatively compact, elliptical morphology. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population within the core. Moving outward from the core, the light gradually diminishes, indicating a smooth decline in stellar density. There is a slight elongation, but generally, the galaxy appears fairly round. The color profile suggests a lack of significant recent star formation, trending towards older stellar populations. There's no readily apparent structure such as spiral arms or a prominent disk. No signs of tidal disturbances or ongoing merger activity are immediately visible, suggesting a relatively isolated system. The galaxy is not particularly blue, rather it has a redder hue.