This galaxy exhibits characteristics indicative of a possible ongoing or recent merger event. The morphology suggests a system with two distinct components. The primary component displays a smooth, elliptical shape, exhibiting a yellowish hue. Juxtaposed to this is a secondary, less defined, bluer component, potentially indicating a region of active star formation. The overall structure is somewhat elongated, deviating from a perfectly spherical morphology. The color differential between the components suggests variations in stellar populations and age. There is evidence that this is a high mass galaxy with on going star formation, given its overall color profile and morphology. The system shows signs of tidal disturbances, albeit not extremely pronounced, which is consistent with a merging or recently merged system. Further spectral analysis is required to confirm the redshift and star formation rates suggested by its color. The galaxy is considered to be large, being an estimated ~13 kpc across.
