The galaxy presents as a blended system comprised of two distinct components. The brighter, primary component exhibits a largely featureless, smooth morphology. The color profile suggests an older stellar population, with a reddish-yellow hue dominating its core, possibly indicating a population of evolved stars and a lack of active star formation. The fainter, secondary component displays a more complex structure. It has a slightly irregular, disk-like appearance, oriented at a shallow angle relative to the primary component. The secondary component shows a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. There appears to be minimal tidal disturbance observed in the image, suggesting any interaction is potentially minor. The galaxy is generally classified as elliptical and is likely not experiencing significant ongoing star formation.
