The galaxy appears as a centrally concentrated, relatively smooth object. Its core is bright, exhibiting a yellowish hue, suggesting a population of older stars. Moving outward from the core, the light fades gradually, and a redder color component becomes visible. There is no readily apparent spiral structure or distinct dust lane. It is a galaxy, with a somewhat elliptical morphology. Indications of star formation are present, though perhaps at a modest rate, the smoothness suggests it is more in the realm of being non-active. No signs of major merger activity are apparent, though the color gradients suggest some mild interactions or disturbances in the past might have occurred. Overall, the galaxy presents as a relatively quiescent system.
