The galaxy appears to be undergoing a merging event, exhibiting multiple distinct luminous components. The primary structure presents a relatively smooth, elliptical morphology, with a high degree of central concentration. A secondary, smaller component is located nearby, potentially interacting gravitationally. Evident color gradients suggest differential stellar populations within the system. The main body exhibits a yellowish-red hue, indicative of older stellar populations, while bluer, fainter regions might be indicative of ongoing, though subdued, star formation. The overall system appears to be in a dynamically disturbed state, deviating from a regular spiral or elliptical form. No prominent spiral arms are discernible. The galaxy displays a moderate redshift.
