The galaxy appears to be a complex system, potentially undergoing an interaction or merger. The primary component exhibits a predominantly smooth, elliptical morphology, characterized by a concentrated central bulge with a yellow/orange hue, suggesting an older stellar population. A secondary, less-defined structure is visible nearby, showing a bluer color, indicative of younger stars or active star formation. This secondary component displays a more irregular form, possibly disrupted due to gravitational interaction. There is little evidence of well-defined spiral arms within either structure, leaning towards a more amorphous or disrupted morphology for both. The overall light profile suggests a system dominated by an evolved population within the primary component, with pockets of ongoing or recent star formation in the secondary or interacting component. The system has signs of disturbance.
